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Sample records for cordeiros morada nova

  1. Avaliação dos fatores ambientais no desenvolvimento corporal de cordeiros deslanados da raça Morada Nova Environmental effects on growth rate of Morada Nova hair lambs in Northeastern Brazil

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    Antônio Amaury Oriá Fernandes

    2001-10-01

    Full Text Available Foram analisados registros de um rebanho de ovinos da raça Morada Nova, coletados num período de 11 anos (1981 a 1991, com o objetivo de avaliar os efeitos de ambiente sobre as características de crescimento dos cordeiros. Os efeitos de ano de nascimento (A, sexo do cordeiro (S, tipo de nascimento (T e peso da ovelha ao parto (P foram importantes fontes de variação para explicar as diferenças nos pesos corporais ao nascimento (PN, ao desmame (PD, aos seis meses (PM6 e aos 12 meses de idade (PM12. Os cordeiros machos foram mais pesados que as fêmeas em todas as idades estudadas. Cordeiros nascidos e criados como simples (SS pesaram mais que os nascidos duplos e criados como simples (GS e os nascidos e criados como duplos (GG. A idade da ovelha (I teve efeito significativo sobre PN, PD e PM6. Concluiu-se que práticas de manejo alimentar devem ser utilizadas para reduzir os efeitos dos fatores ambientais, como ano de nascimento, tipo de nascimento e peso da matriz ao parto, no desenvolvimento corporal dos cordeiros. Fatores de ajuste para sexo do cordeiro, tipo de nascimento e idade da ovelha devem ser estimados e considerados em programas de seleção, a fim de avaliar melhor o crescimento dos cordeiros da raça Morada Nova.Records from an unselected flock of Morada Nova sheep collected over an 11-year period (1981 to 1991 were used to evaluate environmental sources of variation affecting growth traits. The effects of year of birth to yearling (A, sex of lamb (S, type of birth (T, and weigth of ewe at lambing (P were important sources of variation to explain differences in weigth at birth (PN, weaning (PD, six- months (PM6 and 12 months (PM12 of age. Males were heavier than female lambs at all ages. Single lambs born and raised as singles (SS weighed more at all ages than twins raised as singles (GS or twins raised as twins (GG. Age of ewe at lambing (I had a significant effect on PN, PD, and PM6. Results suggest that nutritional

  2. Effects of dietary energy density on nutrient digestibility, performance and carcass characteristics of Morada Nova lambsEfeitos da densidade de energia da dieta sobre a digestibilidade dos nutrientes, o desempenho e as características de carcaça de cordeiros Morada Nova

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    Marcus Roberto Goes Ferreira Costa

    2013-06-01

    Full Text Available Effects of metabolizable energy (ME levels were evaluated on nutrient digestibility and carcass characteristics in Morada Nova lambs. Forty Morada Nova lambs with initial weight of 12.2 ± 2.05 kg, were used. Five treatments were defined according to metabolizable energy (0.96; 1.28; 1.72; 2.18 and 2.62 Mcal/kg DM levels. It was used a randomized block design. Animals were slaughtered when body weight mean (BW of the group reached 25 kg. Linear effect was observed for digestibility coefficient of DM, OM, EE, CP, NDF, TC, FC and NFC. Daily weight gain (DWG presented linear increase (P Foram avaliados os efeitos de diferentes níveis de energia metabolizável (EM sobre a digestibilidade e características de carcaça em cordeiros Morada Nova. Utilizaram-se 40 cordeiros Morada Nova, com peso inicial de 12,2 ± 2,05 kg. Cinco tratamentos foram definidos de acordo com os níveis de energia metabolizável (0,96; 1,28; 1,72; 2,18 e 2,62 Mcal/kg MS, conduzidos em delineamento de blocos ao acaso. Os animais foram abatidos quando a média de peso corporal (PC do grupo atingiu 25 kg. Foi observado efeito linear para o coeficiente de digestibilidade da MS, MO, EE, PB, FDN, CT, FC e NFC. O ganho de peso diário (GPD apresentou aumento linear (P<0,0001 com os níveis de EM. O maior GPD observado foi de 135,98 g/dia para o nível de 2,62 Mcal/kg MS. As características de carcaça avaliadas (peso de carcaça quente, peso de carcaça fria, perda por resfriamento em kg e rendimento biológico não variaram em função dos níveis de EM, com valores médios de 11,52; 11,03; 0,48 e 57,25, respectivamente. Conclui-se que o incremento do nível de energia em dietas influencia a digestibilidade dos nutrientes e ganhos de peso diário de cordeiros Morada Nova, durante o período de crescimento, sem alterar as características de carcaça.

  3. Effects of weaning age and weight on lamb growth rate of Morada Nova breed raised in a tropical extensive production system Efeito da idade e do peso ao desmame no ganho de peso de cordeiros Morada Nova criados em sistema extensivo de produção no trópico

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    Arturo Bernardo Selaive -Villarroel

    2008-06-01

    Full Text Available The aim of this research were to study the effect of weaning age and weight on post-growing rate (PWG and to estimate the optimal weaning age (WA and weight (WW of Morada Nova-white variety breed lambs raised under extensive system conditions. A total of 31 male and female lambs were evaluated, being 19 lambs born in April/May 2001 and 12 lambs born in February/March 2002. Lambs were distributed in the following treatments at weaning: 1 weaning age = T1: weaned at 60 days; T2: weaned at 75 days; T3: weaned at 90 days, and 2 weaning weight = T1: weaned with 9 to 10.4kg weigth; T2: weaned with 10.5 to 12.4kg weight and T3: weaned with above 12.5kg weight. The PWG was recorded through successive weightings done every fourteen days from weaning to 180 days of age. Data were analysed through a statistical model that included age and weight at weaning, sex and year of birth as fixed effects. Lambs weaned with 60, 75 and 90 days of age showed non-significant differences (P>0.05 on PWG. However, WW had a significant influence (PO trabalho teve como objetivo avaliar o efeito da idade e do peso ao desmame no ganho de peso posterior de cordeiros da raça Morda Nova-variedade branca, bem como determinar a idade e o peso mais adequados de desmame de cordeiros mantidos em sistema extensivo de criação. Foram avaliados 31 cordeiros machos e fêmeas, sendo 19 nascidos nos meses de abril e maio e 12 nascidos durante os meses de fevereiro e março de 2002. Ao desmame, os cordeiros foram distribuídos nos seguintes tratamentos, considerando-se: 1 idade ao desmame (ID = T1: desmame com 60 dias de idade; T2: desmame com 75 dias de idade; T3: desmame com 90 dias de idade; e 2 peso ao desmame (PD = T1: desmame com peso entre 9 - 10,4kg; T2: desmame com peso entre 10,5 - 12,4; T3: desmame com peso acima ou igual a 12,5kg. O crescimento posterior dos cordeiros foi avaliado através de pesagens sucessivas quinzenais até atingirem a idade de 180 dias. Os dados foram

  4. Características quantitativas da carcaça de cordeiros deslanados Morada Nova em função da relação volumoso:concentrado na dieta Quantitative characteristics of the carcass of Morada Nova lambs fed different dietary ratios of forage and concentrate

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    Severino Gonzaga Neto

    2006-08-01

    Full Text Available Com o objetivo de avaliar a influência da relação volumoso:concentrado sobre a composição tecidual e os rendimentos de carcaça e de cortes comerciais de cordeiros Morada Nova em confinamento, utilizaram-se 18 cordeiros com peso vivo (PV inicial de 15 kg, distribuídos em seis grupos de três animais (um em cada dieta, de acordo com a relação volumoso(V:concentrado(C: 40:60, 55:45 e 70:30. Foram avaliados os pesos de corpo vazio (PCV, de carcaça quente (PCQ e de carcaça fria (PCF, a partir dos quais foram calculados os rendimentos biológico (RB, de carcaça quente (RCQ e de carcaça fria (RCF e a perda de peso por resfriamento (PPR. A carcaça foi dividida em cinco cortes cárneos (perna, lombo, costelas, paleta e pescoço, os quais foram pesados para cálculo de seus rendimentos em relação ao peso da meia-carcaça. A perna foi dissecada em músculo, osso e gordura e os pesos desses tecidos foram expressos em peso absoluto e em porcentagem da perna. Calcularam-se as relações músculo:osso e músculo:gordura, o índice de musculosidade da perna (IMP e a área de olho-de-lombo (AOL. O aumento de 30 para 60% de concentrado na dieta elevou os rendimentos de carcaça quente e carcaça fria, assim como o rendimento biológico. Os crescentes teores de concentrado na dieta não afetaram a porcentagem de músculo na perna, mas proporcionaram maior deposição de gordura e maior área de olho-de-lombo.Eighteen lambs averaging initial body weight (BW of 15 kg were allotted to six groups of three animals (one lamb per diet and were fed diets with following forage:concentrate ratios (F:C: 1 40F:60C; 2 55F:45C; or 3 70F:30C. Lambs of each group were slaughtered when the animal fed the diet with the highest concentrate level reached 25 kg of BW. Animals were slaughtered after 16 h of fasting (feed and water. After obtaining the slaughter body weight (SBW, animals were anesthetized by electric discharge and killed by bleeding of the carotid

  5. Efeito dos níveis de concentrado sobre o desempenho de ovinos Morada Nova em confinamento Effect of concentrate level on performance of feedlot Morada Nova sheep

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    Geovergue Rodrigues de Medeiros

    2007-08-01

    Full Text Available Avaliaram-se o desempenho e a digestibilidade dos nutrientes em 32 ovinos Morada Nova, castrados, em confinamento alimentados com dietas contendo 20, 40, 60 e 80% de concentrado. Os animais tinham 8,11 ± 1,15 meses de idade, peso inicial de 19,67 ± 2,97 kg e peso ao abate de 30,0 kg. Utilizou-se delineamento experimental em blocos casualizados, com quatro tratamentos e oito repetições. Houve efeito linear decrescente dos níveis de concentrado sobre o número de dias em confinamento, que variou de 123,37 a 52,50 para as dietas com 20 e 80% de concentrado. O consumo diário de MS aumentou linearmente com a redução da proporção volumoso:concentrado, que variou de 0,925 a 1,124 kg. O ganho de peso, a conversão e a eficiência alimentar melhoraram com aumento do nível de concentrado na dieta. Os consumos de MO, PB, EE, NDT, EM, carboidratos totais (CT e carboidratos não-fibrosos (CNF elevaram, enquanto os de FDN e FDA decresceram com a inclusão do concentrado. Os coeficientes de digestibilidade de MS, MO e dos CT foram crescentes, enquanto a digestibilidade do EE e dos CNF sofreram efeito quadrático e as digestibilidades de PB, FDN e FDA não foram influenciadas pelo aumento de concentrado na dieta. Níveis de concentrado acima de 60% elevaram os ganhos de peso e anteciparam a idade ao abate dos ovinos Morada Nova. Dietas com níveis superiores a 40% de concentrado melhoraram os índices de digestibilidade aparente dos nutrientes. A raça Morada Nova tem potencial para produção de carne em confinamento.The objective of this trial was to evaluate performance and nutrient intake and digestibility in feedlot Morada Nova hair sheep fed increasing levels of dietary concentrate. Thirty-two castratated Morada Nova sheep averaging 8.11 ± 1.15 months of age and 19.67 ± 2.97 kg of body weight (BW at the beginning of the study were used in this trial. Animals were slaughtered with 30.0 kg of BW and fed diets with the following concentrate

  6. Relação materno-filial da raça Morada Nova recebendo dietas com três níveis de energia, ao final da gestação Ewe-lambs relationship in Morada Nova breed under three energy levels at the end of gestation

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    Tobyas Maia de Albuquerque Mariz

    2007-12-01

    Full Text Available Objetivou-se com este trabalho avaliar os efeitos de diferentes níveis de energia ofertados no terço final da gestação sobre o comportamento materno-filial de animais da raça Morada Nova. O experimento consistiu de três tratamentos - três grupos de oito matrizes, alimentadas com dietas isoprotéicas contendo diferentes níveis energéticos (2,0; 2,4 e 2,8 Mcal EM/kg MS, com oito repetições cada. Observou-se efeito dos tratamentos sobre as variáveis comportamentais maternas avaliadas (vocalização, ato de cheirar e lamber a cria e a posição da ovelha em - pé ou deitada, nas ovelhas, mas não foi observada diferença para os comportamentos filiais (posição da cria, tempo decorrido do nascimento à primeira vez que ficou de pé, tempo decorrido do nascimento à primeira mamada, tempo total de mamadas dos cordeiros. A mobilização de reservas ou o carreamento direto de nutrientes da dieta para o crescimento fetal normal, nos grupos alimentos com dietas contendo 2,0 e 2,4 Mcal EM/kg MS, minimizaram os possíveis efeitos sobre o comportamento filial dos cordeiros. Mesmo sob interferência no relacionamento com as crias, ovelhas Morada Nova conseguiram manter as condições dos cordeiros inalteradas em todos os tratamentos.The present work was carried out with the objective to evaluate the effects of different energy levels offered in the final third of gestation on the ewe-lambs behavior of animals from the Morada Nova breed. The experiment was divided into three treatments - three groups of eight ewes, fed isoprotein diets containing different energy levels (2.0, 2.4, and 2.8 Mcal ME/kg DM, with eight replicates each. There was effect of the treatment on the maternal behavior evaluated variables (vocalization, act of smell and lick the lambs and the position of the ewe - stand up or lying, in the ewes, but no difference was observed for the filial behavior (position of animal, time from the birth to the first time that the animal was

  7. Reproductive parameters on hair sheep (Morada Nova and Santa Inês reared in intensive systems in Southeastern Brazil

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    André Torres Geraldo

    2013-12-01

    Full Text Available In southeastern Brazil, the Santa Inês ewes is one of the most used to produce early slaughtering crossbred lambs. The Morada Nova breed is reared only in some regions of Brazil and has a very small number of animals and flocks, but ewes have potential to be used for lamb production in the southeast, due to their adaptability to tropical conditions. This experiment aims to evaluate the reproductive potential of Morada Nova ewes to produce early lambs for slaughter. The study was carried out at Instituto de Zootecnia, city of Nova Odessa, located in São Paulo State, Brazil. Forty-nine adult Santa Inês (SI ewes with 51.8 ± 7.07 kg of initial body weight and forty-nine Morada Nova (MN with 33.1 ± 4.98 were used. During pregnancy the ewes were reared on intensive grazing systems with rotational grazing on Aruana grass pasture (Panicum maximum cv.IZ-5, and in the final third of gestation received corn silage ad libitum and a concentrate mixture (400 g/day with 16% crude protein and 80% of total digestible nutrient (TDN. The length of pregnancy, calculated through the date of mating and date of birth; prolificacy rate obtained by the number of lambs born per ewes; percentage of multiple births (% and ewe’s weight at lambing (kg were calculated. Statistical analysis was carried using GLM procedure of SAS ®. The birth weight of MN ewes was lower than the SI ewes, which is a reflection of their smaller size, however, the other reproductive parameters were similar between genotypes. These results highlight the potential use of Morada Nova ewes, as smaller maternal breed, for lamb production, which is favorable for production system that seeks sustainable intensification and optimization of resources, especially food.

  8. Carcass and meat traits of Morada Nova, Santa Ines and ½ Ile de France ½ Texel lambs finished in feedlot

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    Juliano Issakowicz

    2014-03-01

    Full Text Available The aim of this study was to evaluate the carcass and meat traits of Morada Nova, Santa Ines and ½ Ile de France ½ Texel lambs finished in feedlot. Weight and proportion of meatcuts, measures of carcass size and color, tenderness, cooking loss and ultimate pH of meat from 10 Morada Nova, 6 Santa Ines and 10 ½ Ile de France ½ Texel were evaluated. The lambs were finished in collective pens, fed ad libitum with 50% corn silage and 50% concentrate and slaughtered at about six months old. Analysis of variance was performed by the procedure PROC GLM of SAS (SAS Inst., Inc., Cary, NC and means were compared by Tukey test at 5% significance. The Morada Nova lambs had values of 14.1 kg, 13.9 kg, 0.240 kg/cm, 56.2 cm and 35.8 cm for hot and cold carcass weight, compactness index, hip and leg circumference respectively and these values were lower (P <0.05 to values observed in Santa Ines (19.4 kg, 18.8 kg, 0.283 cm/kg, 64.6 cm and 40.0 cm and in ½ Ile de France ½ Texel (18.6 kg, 18.2 kg, 0.305 cm/kg; 65.4 cm and 41.6 cm lambs. The hot and cold carcass yield did not differ (P> 0.05 among genetic groups. The scores for conformation and fat cover were higher (P <0.05 in ½ Ile de France ½ Texel lambs (2.4 and 3.0 and the carcass length was greater in Santa Ines lambs (66.3 cm. The ½ Ile de France ½ Texel lambs had smaller (P<0.05 proportion of neck and greater of leg (9.10% and 33.1% compared to Morada Nova lambs (10.3% and 30.4% and Santa Inês (10.9% and 31.6%. The weight of shoulder, leg, rack, ribs and flank was lower (P<0.05 in Morada Nova (1.306, 2.127 kg, 0.999 kg, 0.775 kg and 0.433 kg respectively compared to Santa Inês (1.820 kg, 2.972 kg, 1.355 kg, 0.959 and 0.509 kg and ½ Ile de France ½ Texel (1.791 kg, 3.007 kg, 1.212 kg, 1.016 kg and 0.563 kg. The neck was heavier in Santa Ines (1.038 kg which differed (P <0.05 from the other genetic groups (0.725 kg for Morada Nova and 0.830 kg for ½ Ile de France x ½ Texel lambs. The ½ Ile de

  9. Diagnosis of subclinical mastitis in Santa Inês and Morada Nova sheep in southeastern Brazil.

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    Zafalon, Luiz Francisco; Santana, Raul Costa Mascarenhas; Pilon, Lucas Eduardo; Júnior, Guilherme Aparecido Fim

    2016-06-01

    The objective of this study was to evaluate different screening limits for the California mastitis test (CMT) and the somatic cell count (SCC) in previous diagnoses of subclinical mastitis in Santa Inês and Morada Nova ewes, which were reared under the same management conditions. Additionally, cutoff points were defined for SCC in accordance with the sensitivity and specificity of the test. A total of 907 mammary halves were subjected to CMT and SCC. The disease was confirmed by means of microbiological identification. Coagulase-negative staphylococci (CNS) were the microorganisms with highest occurrence. The CMT score of 1+ provided adequate sensitivity and specificity at all periods of lactation investigated. This score showed good agreement with SCC, >400,000 cells mL(-1). Higher cell counts favored higher diagnostic specificity. They can be used when producers have financial difficulties relating to treatment or culling of sheep with subclinical mastitis. However, producers should be warned about the risk of false-negative results in the flock.

  10. Traditional and alternative nonlinear models for estimating the growth of Morada Nova sheep

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    Laaina de Andrade Souza

    2013-09-01

    Full Text Available In the present study, alternative and traditional nonlinear models to describe growth curves of Morada Nova sheep reared in the state of Bahia, Brazil, were applied. The nonlinear models were: Schnute, Mitscherlich, Gompertz, Logistic, Meloun I Meloun II, III Meloun, Gamito and Meloun IV. The model adjustment was evaluated by using: Adjusted Coefficient of Determination (R²aj, Akaike Information Criterion (AIC, Bayesian Information Criterion (BIC, Mean Squared Error of Prediction (MEP and Coefficient of Determination of Prediction (R²p. The selection of the best model was based on cluster analysis, using the evaluators as variables. Six out of the nine tested models converged, while Meloun I and Meloun IV were equally effective in explaining animal growth, without significant influence of sex or type of parturition over the curve parameters. The models Meloun I and IV have the best adjustment and reveal a remarkable reduction of weight gain after 150 days of age, which indicates special attention should be given to feeding at this stage.

  11. Respiratory heat loss in Morada Nova sheep in Brazilian semi-arid regions

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    Steffan Edward Octávio Oliveira

    2013-07-01

    Full Text Available This study aimed to evaluate the respiratory heat loss in sheep from the equations developed for this species and its relations with meteorological variables in semi-arid regions. The respiratory heat loss (sensible and latent was estimated through the equations in the literature for four 12-month-old male Morada Nova sheep, kept in an installation with shading of ceramic tiles and a 3-meter-high ceiling. The following environmental variables were measured: air temperature (TA, wind speed (U, relative humidity (RH and partial vapor pressure (PP{tA}. The physiological variables measured: rectal temperature (TR and respiratory rate (RR. Statistical analysis was performed based on regression using PROC REG procedure in SAS. The latent respiratory heat loss showed a linear and positive correlation with ambient temperature. However, the respiratory convection showed a linear and negative correlation, but with incipient values. Therefore, the latent heat loss is more important than the sensible one in the respiratory system to maintain thermoregulation of sheep in a semi-arid region of Brazil.

  12. Genetic diversity and population structure of different varieties of Morada Nova hair sheep from Brazil.

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    Ferreira, J S B; Paiva, S R; Silva, E C; McManus, C M; Caetano, A R; Façanha, D A E; de Sousa, M A N

    2014-01-01

    The aim of this study was to analyze genetic diversity and population structure among varieties of White (N = 40), Red (N = 32), and Black (N = 31) Morada Nova hair sheep from flocks in the northeastern Brazilian semiarid region. Fifteen nuclear microsatellite markers and two regions of mitochondrial DNA were used. The intra-population analysis demonstrated that the White variety had higher diversity, while the Red variety had the lowest values. The Bayesian analysis to assess the genetic population structure allowed differentiation between White, Red, and Black varieties, and revealed a tendency towards sub-structuring in the White variety flocks from the States of Ceará and Paraíba. The results of analyses of molecular variance showed that the greatest genetic structure was found when comparing flocks rather than varieties (8.59 vs 6.64% of the total variation, P Dtl, both the dendrogram analysis and the principal coordinate analysis showed the formation of two main groups: one composed of White and another of Black and Red individuals. Five and two haplotypes were found for the D-loop region and the ND5 gene, respectively. A haplotype unique to the Red variety was found in the D-loop region and a variety haplotype unique to the Black variety was found in the ND5 gene; however, these frequencies were low and therefore require further validation. These results support the existence of substantial differences between the Red and White varieties and should be used as separate genetic resources and to improve conservation programs.

  13. Desempenho reprodutivo de ovelhas morada nova submetidas a induÃÃo do estro pelo efeito macho

    OpenAIRE

    2013-01-01

    O presente trabalho teve como objetivo principal avaliar a eficiÃncia do efeito macho como mÃtodo indutivo da atividade estral em trÃs categorias (NulÃparas, PrimÃparas e PlurÃparas) de fÃmeas ovinas mestiÃas (MORADA NOVA X SPRD), e no desempenho reprodutivo, a partir de dados obtidos de manifestaÃÃo de estro; intervalo entre a introduÃÃo do macho e o inÃcio do estro; grau de sincronizaÃÃo; repetiÃÃo de estros; taxa de prenhez; taxa de partos; taxa de gemelaridade e Ãndice de prolificidade. E...

  14. Models to predict both sensible and latent heat transfer in the respiratory tract of Morada Nova sheep under semiarid tropical environment

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    Fonseca, Vinícius Carvalho; Saraiva, Edilson Paes; Maia, Alex Sandro Campos; Nascimento, Carolina Cardoso Nagib; da Silva, Josinaldo Araújo; Pereira, Walter Esfraim; Filho, Edgard Cavalcanti Pimenta; Almeida, Maria Elivânia Vieira

    2016-10-01

    The aim of this study was to build a prediction model both sensible and latent heat transfer by respiratory tract for Morada Nova sheep under field conditions in a semiarid tropical environment, using easily measured physiological and environmental parameters. Twelve dry Morada Nova ewes with an average of 3 ± 1.2 years old and average body weight of 32.76 ± 3.72 kg were used in a Latin square design 12 × 12 (12 days of records and 12 schedules). Tidal volume, respiratory rate, expired air temperature, and partial vapor pressure of the expired air were obtained from the respiratory facial mask and using a physiological measurement system. Ewes were evaluated from 0700 to 1900 h in each day under shade. A simple nonlinear model to estimate tidal volume as a function of respiratory rate was developed. Equation to estimate the expired air temperature was built, and the ambient air temperature was the best predictor together with relative humidity and ambient vapor pressure. In naturalized Morada Nova sheep, respiratory convection seems to be a mechanism of heat transfer of minor importance even under mild air temperature. Evaporation from the respiratory system increased together with ambient air temperature. At ambient air temperature, up to 35 °C respiratory evaporation accounted 90 % of the total heat lost by respiratory system, on average. Models presented here allow to estimate the heat flow from the respiratory tract for Morada Nova sheep bred in tropical region, using easily measured physiological and environmental traits as respiratory rate, ambient air temperature, and relative humidity.

  15. Models to predict both sensible and latent heat transfer in the respiratory tract of Morada Nova sheep under semiarid tropical environment

    Science.gov (United States)

    Fonseca, Vinícius Carvalho; Saraiva, Edilson Paes; Maia, Alex Sandro Campos; Nascimento, Carolina Cardoso Nagib; da Silva, Josinaldo Araújo; Pereira, Walter Esfraim; Filho, Edgard Cavalcanti Pimenta; Almeida, Maria Elivânia Vieira

    2017-05-01

    The aim of this study was to build a prediction model both sensible and latent heat transfer by respiratory tract for Morada Nova sheep under field conditions in a semiarid tropical environment, using easily measured physiological and environmental parameters. Twelve dry Morada Nova ewes with an average of 3 ± 1.2 years old and average body weight of 32.76 ± 3.72 kg were used in a Latin square design 12 × 12 (12 days of records and 12 schedules). Tidal volume, respiratory rate, expired air temperature, and partial vapor pressure of the expired air were obtained from the respiratory facial mask and using a physiological measurement system. Ewes were evaluated from 0700 to 1900 h in each day under shade. A simple nonlinear model to estimate tidal volume as a function of respiratory rate was developed. Equation to estimate the expired air temperature was built, and the ambient air temperature was the best predictor together with relative humidity and ambient vapor pressure. In naturalized Morada Nova sheep, respiratory convection seems to be a mechanism of heat transfer of minor importance even under mild air temperature. Evaporation from the respiratory system increased together with ambient air temperature. At ambient air temperature, up to 35 °C respiratory evaporation accounted 90 % of the total heat lost by respiratory system, on average. Models presented here allow to estimate the heat flow from the respiratory tract for Morada Nova sheep bred in tropical region, using easily measured physiological and environmental traits as respiratory rate, ambient air temperature, and relative humidity.

  16. Productive traits of Santa Inês and Morada Nova ewes mated with Dorper rams in Southeastern Brazil

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    André Torres Geraldo

    2013-12-01

    Full Text Available Naturalized Brazilian hair breeds are adapted to tropical climate, however produce lambs for slaughter with lower performance and carcass traits. One way to increase productiveness comprises the use of adapted ewes crossed with specialized meat breeds, exploiting the complementarity between breeds and heterosis for sustainable lamb production. Dorper rams can be use to produce crossbred lambs with better performance traits. The aim of this study was to evaluate the weight at birth and at 30 days of Morada Nova lambs (MN and Santa Inês (SI straight breed or Dorper crossbred. The study was carried out at Instituto de Zootecnia, city of Nova Odessa, located in São Paulo State, Brazil. Forty-two adult Santa Inês (SI ewes with 51.8 ± 7.1 Kg of initial body weight, with 21 mated with SI rams and 21 mated with Dorper (DO rams and 38  Morada Nova (MN with 33.1 ± 4.98 with 19 mated with MN and  19 mated with DO rams were used. During pregnancy the ewes were reared on intensive grazing systems with rotational grazing on Aruana grass (Panicum maximum cv. Aruana, plus corn silage ad libitum and a concentrate mixture (400 g/day with 16% crude protein and 80% of total digestible nutrient (TDN on  final third of gestation. After lambing, the ewes were kept in collective pens and kept under the same diet used in late pregnancy. The weight at birth as well as at 30 day old were recorded and calculated the percentage of lamb weight in relation of ewe weights. Statistical analyses were performed using SPSS software version 12. Based on data is possible to observe that the SI X DO lambs had the highest birth weight followed by the straight breed SI and MN. At 30 day, the SI lambs had greater live weight than MN lambs. No difference was found for lamb´s weights in relation to ewe’s weight. We conclude that SI crossbred or straight breed lambs are heavier than MN ones.

  17. Efeitos de dieta contendo castanha de caju sobre o desenvolvimento ponderal, parÃmetros seminais e proteoma do plasma seminal de carneiros Morada Nova

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    Emerson Pinto Moreira

    2015-01-01

    O presente estudo avaliou os efeitos da inclusÃo de 13% de farelo de castanha de caju (CNM) na dieta de carneiros Morada Nova nos parÃmetros seminais e proteÃnas do plasma seminal. Vinte carneiros foram distribuÃdos em dois grupos iguais: grupo castanha de caju (CNG) e grupo controle (COG). O CNG e COG receberam 13% e 0% de CNM na dieta durante 90 dias. Os grupos foram comparados para peso corporal, circunferÃncia escrotal, parÃmetros seminais e proteÃnas do plasma seminal, utilizando o MÃtod...

  18. Composição centesimal e análise sensorial da carne de ovinos Morada Nova alimentados com dietas contendo melão em substituição ao milho Centesimal composition and sensorial analysis of Morada Nova lambs fed diets containing melon fruit in substitution of corn grain

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    Roberto Germano Costa

    2011-12-01

    Full Text Available Objetivou-se avaliar a influência da adição de melão em substituição ao milho moído em dietas sobre a composição centesimal e análise sensorial da carne de ovinos da raça Morada Nova. Foram utilizados 20 animais da raça Morada Nova, machos não-castrados, com peso vivo médio inicial de 15 kg, distribuídos em delineamento inteiramente ao acaso para avaliação de quatro níveis (0, 30, 60 e 100% de inclusão de melão em substituição ao milho moído, cada um avaliado com cinco repetições. Para determinar a composição centesimal da carne, utilizou-se o músculo semimembranosus. Com o músculo longissimus dorsi, procedeu-se à análise sensorial quantificando, por intermédio de notas, os atributos de sabor, odor, suculência, maciez e aparência global. As análises dos dados não apresentaram diferenças significativas para a composição centesimal (umidade, proteína, lipídio e matéria mineral. Na análise sensorial, a suculência apresentou comportamento quadrático, com ponto de máximo de 5,18, e as demais qualidades organolépticas (odor, sabor, maciez e aparência global não foram influenciadas pela inclusão de melão em substituição ao milho nas dietas. A utilização de melão em substituição ao milho em dietas para ovinos Morada Nova não afeta as principais qualidades organolépticas da carne.The objective of this trial was to evaluate the influence of the addition of melon fruit replacing ground corn in diets on the centesimal composition and sensory analysis of meat from Morada Nova lambs. Twenty Morada Nova males with average weight of 15 kg were distributed in a completely randomized design with four increasing levels (0, 30, 60 and 100% of melon in substitution of ground corn, each one with five replications. To determine the chemical composition of meat, the semimembranosus muscle was used. With the muscle longissimus dorsi sensory analysis, the attributes of taste, odor, juiciness, softness and

  19. Weight and yield of non-carcass components of Morada Nova lambs fed with different levels of metabolizable energyPeso e rendimento dos componentes não-carcaça de ovinos Morada Nova alimentados com diferentes níveis de energia metabolizável

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    Danilo de Araújo Camilo

    2012-12-01

    Full Text Available The objective of this study was to evaluate the effect of different metabolizable energy (ME levels on weight of gastrointestinal content, weight and yield of the internal organs and gastrointestinal compartments of Morada Nova growing lambs. Thirty-two animals, non-castrated, with average body weight of 12.12 ± 1.69 kg and two months old approximately, were used. The animals were distributed into four different metabolizable energy (1.28; 1.72; 2.18 and 2.62 Mcal/kg DM levels, in randomized block design with eight replicates per treatment. Tifton 85 hay was used as roughage. There was no effect of energy levels (P > 0.05 on weight of gastrointestinal content. Increased linear effect (P Objetivou-se com o presente estudo avaliar o efeito de diferentes níveis de energia metabolizável (EM sobre: peso do conteúdo do trato gastrintestinal, peso e rendimento dos órgãos internos e compartimentos gastrintestinais em ovinos Morada Nova em crescimento. Foram utilizados 32 animais, não castrados, com peso corporal médio de 12,12 ± 1,69 kg e, aproximadamente, dois meses de idade. Os animais foram distribuídos em quatro diferentes níveis de EM (1,28; 1,72; 2,18 e 2,62 Mcal/kg de MS, em delineamento em blocos casualizados, com oito repetições por nível de EM. O feno de Tifton 85 foi utilizado como volumoso. Não foi observado efeito (P > 0,05 dos níveis de energia sobre o peso do conteúdo gastrintestinal. Verificou-se efeito linear crescente (P < 0,05 dos níveis de EM sobre os pesos do coração, PTEL (pulmões, traqueia, esôfago e língua, fígado e baço, expressos em kg. Em relação aos compartimentos do trato gastrintestinal foi observado efeito linear crescente (P < 0,05 dos níveis de EM somente sobre o rúmen-retículo, em %, e intestino delgado, em kg. As gorduras perirrenal, omental e mesentérica foram influenciadas pelos níveis de EM (P < 0,05, com incremento linear para os pesos em kg e %. O aumento dos níveis de EM das ra

  20. Efeito de níveis de melão em substituição ao milho moído sobre o desempenho, o consumo e a digestibilidade dos nutrientes em ovinos Morada Nova Effect of melon in substitution of ground corn on performance, intake, and nutrients digestibility in Morada Nova lambs

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    Cláudio Adriano Correia de Lima

    2012-01-01

    Full Text Available Avaliaram-se o desempenho, o consumo e a digestibilidade aparente de componentes nutritivos em 32 ovinos Morada Nova em confinamento, 20 machos não-castrados e 12 fêmeas, recebendo dietas contendo 0, 30, 60 e 100% de melão em substituição ao milho moído. Os animais tinham em média 6 meses de idade, peso médio inicial de 15 kg e foram abatidos aos 25 kg. Utilizou-se delineamento experimental inteiramente casualizado, com quatro tratamentos e oito repetições. O consumo de MS apresentou tendência quadrática para ambos os sexos, variando de 769 a 837 g para os machos e de 722 g a 646 g para as fêmeas. Os consumos de matéria orgânica (MO, proteína bruta (PB, extrato etéreo (EE, fibra em detergente neutro (FDN, nutrientes digestíveis totais (NDT, carboidratos totais (CT e carboidratos não-fibrosos (CNF apresentaram comportamento quadrático, refletindo o mesmo comportamento da ingestão da MS. A digestibilidade aparente da MS apresentou tendência linear decrescente. Os coeficientes de digestibilidade aparente de MO, PB, EE, FDN e CT apresentaram comportamento linear crescente com a adição de melão em substituição ao milho moído. O ganho de peso diário com o aumento do nível de melão na dieta foi maior nos machos. A conversão e eficiência alimentar não foram influenciadas pelo aumento do nível de melão na dieta. Os dias de confinamento variaram de 79 a 90 dias. A substituição na dieta do milho moído por melão possibilitou obter desempenho satisfatório em ovinos Morada Nova em confinamento. O nível de 60% de substituição é o que permite melhor retorno financeiro, entretanto, em níveis superiores a 30%, aumentam os dias de confinamento, elevando a idade ao abate.Performance, intake, and nutrients digestibility of 32 Morada Nova confined lambs were evaluated, using diets with increasing levels (0, 30, 60, 100% of melon (Cucumis melo L. in substitution of corn grain. Animals were about 6 months old, with an

  1. Efeito do flushing sobre o desempenho reprodutivo de ovelhas Morada Nova e Santa Inês submetidas à inseminação artificial em tempo fixo

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    F.P. Gottardi

    2014-04-01

    Full Text Available O objetivo do estudo foi analisar o efeito do flushing, do protocolo hormonal para sincronização de estro e da IATF sobre o desempenho reprodutivo de ovelhas Morada Nova (MN e Santa Inês (SI. Foram utilizadas 27 ovelhas SI e 24 ovelhas MN suplementadas com concentrado (1% do peso vivo, em média durante 75 dias de estação reprodutiva. Após 30 dias de suplementação, as ovelhas foram sincronizadas com protocolo hormonal (PH à base de progestágeno, eCG e cloprostenol. A observação de estro foi realizada após 12, 24, 36 e 48 horas do término do PH, com o auxílio de dois rufiões, e a IATF foi realizada aproximadamente 55 horas após o final do PH. Do 20º ao 45º dia após o início do PH, realizou-se o repasse com um reproduto Dorper. O diagnóstico de prenhez foi realizado 70 dias após a IATF. Foi analisado o peso, escore da condição corporal (ECC, taxa de apresentação de estro, taxa de prenhez e prolificidade, testando-se os efeitos da raça, semana de suplementação (SS e classe de ECC. O peso e ECC das ovelhas variaram em função da SS. Foi observada taxa de estro de 88,2%, sendo que 43,2% das ovelhas apresentaram estro até 24 horas do final do PH. A taxa de prenhez por IATF foi de 31,4% e a de prenhez após repasse foi de 50,0%, sendo que a classe de ECC interferiu nas taxas de prenhez. Obteve-se maior porcentagem de partos múltiplos de ovelhas prenhes por IATF do que por monta natural no repasse. Conclui-se que o flushing resultou em ganho de peso e aumento do ECC, o que garantiu a padronização do rebanho para a estação reprodutiva e, consequentemente, melhorou o desempenho reprodutivo. O PH utilizado aumentou a prolificidade e adiantou o início do estro; porém, não foi eficiente na sincronização de ovelhas deslanadas.

  2. Desempenho e composição da carcaça de cordeiros deslanados terminados em confinamento com diferentes dietas Performance and carcass composition of shorn lambs finished in a feedlot on different diets

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    José Teodorico de Araújo Filho

    2010-02-01

    Full Text Available Este trabalho foi realizado com os objetivos de avaliar os efeitos da alimentação e do genótipo sobre as características quantitativas de carcaça de cordeiros terminados em confinamento e estimar sua margem bruta. Foram utilizados 18 cordeiros de cada genótipo: Morada Nova, Santa Inês e mestiços Dorper × Santa Inês. As rações foram constituídas de 2,5 Mcal EM/kg MS e 2,94 Mcal EM/kg MS. Utilizou-se um delineamento inteiramente casualizado, em esquema fatorial 3 × 2. As dietas influenciaram o ganho de peso diário, o peso de corpo vazio, o escore corporal, a eficiência alimentar e o tempo de confinamento, enquanto o genótipo promoveu diferenças em todas as variáveis estudadas. A densidade calórica das dietas influenciou os rendimentos biológicos, de carcaça quente e fria, esses dois últimos influenciados pelos genótipos. A dieta mais energética (2,94 Mcal EM/kgMS proporcionou maiores pesos absolutos de pescoço, paleta, costela, lombo e perna, porém, em valores relativos, cordeiros alimentados com diferentes níveis energéticos não diferiram quanto a essas características, independentemente do nível energético da dieta. Os rendimentos percentuais dos cortes foram influenciados pelos genótipos, exceto o corte pescoço. Os pesos de todos os cortes foram influenciados pelos genótipos. A maior margem bruta de carcaça foi obtida com ração de maior nível energético.This study was performed with the objective of assessing the effects of feed and genotype on the quantitative characteristics of carcasses of lambs finished in a feedlot and estimate gross margins. Eighteen lambs of each genotype were used: Morada Nova, Santa Inês and cross-breed Dorper × Santa Inês. Feeds with low and high energetic levels consisted of 2.5 Mcal ME/kg DM and 2.94 Mcal ME/kg DM, respectively. A randomized complete design was used, with a 3 × 2 factorial scheme. The diets influenced daily weight gain, empty body weight, body score, feed

  3. Parâmetros de qualidade da carne de cordeiros submetida aos processos de maturação e injeção de cloreto de cálcio Quality parameters of aged and calcium chloride injected lamb meat

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    Nivea Maria Brancacci Lopes Zeola

    2006-10-01

    Full Text Available Foram estudados o pH e a temperatura dos músculos Biceps femoris, Longissimus e Triceps brachii de cordeiros "Morada Nova", durante o período de instalação do rigor mortis, e os efeitos da maturação e da injeção de cloreto de cálcio nas características qualitativas destes músculos. Os cordeiros foram abatidos ao atingirem 25kg de peso vivo. O declínio do pH e da temperatura dos músculos foram monitorados durante a instalação do rigor mortis nos tempos 0, 2, 4, 6, 8, 10, 12 e 24 horas após o abate, com as carcaças refrigeradas em câmara fria a 4°C. Após este período, os músculos foram retirados e submetidos aos respectivos tratamentos com posterior determinação da perda de peso durante a cocção e da maciez. A queda do pH para os músculos Biceps femoris e Longissimus mostrou-se dentro da faixa considerada normal para carne ovina, enquanto o músculo Triceps brachii apresentou pH, às 10, 12 e 24 horas, considerado acima da faixa descrita. O declínio da temperatura apresentou-se típico de condições de resfriamento habituais. O tempo de maturação e a injeção de cloreto de cálcio não afetaram a perda de peso durante a cocção. Em relação à maciez, o tempo de maturação nos músculos Biceps femoris e Longissimus propiciou carne mais tenra e a concentração de 0,3M de cloreto de cálcio melhorou a maciez do músculo Longissimus.Temperature and pH of Biceps femoris, Longissimus and Triceps brachii muscles from ‘Morada Nova' lambs during the rigor mortis and the effects of ageing and calcium chloride injection in qualitative characteristics of these muscles were studied. The lambs were slaughtered with 25kg live weight. The decline of pH and temperature of muscles were monitored during the onset of rigor mortis in times 0, 2, 4, 6, 8, 10, 12 and 24 hours after slaughter, with the carcasses refrigerated at 4°C. The muscles were removed and submitted to respective treatments with determination of cooking loss

  4. António Reis and Margarida Cordeiro, eccentric filmmakers

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    Lucas Tavares Neves

    2016-02-01

    Full Text Available The international symposium "António Reis and Margarida Cordeiro, eccentric filmmakers" took place in Paris between the 3rd and the 4th of June, 2015. Speakers exchanged on the political, social and poetical aspects of the duo's cinematography, as well as on the reverberations of titles such as Jaime (1974 and Trás-os-montes (1976 on the Portuguese filmic landscape of the decades that followed.

  5. Novae news

    CERN Multimedia

    2012-01-01

    As announced in the previous Bulletin, Novae has opened a new snack bar on the Flagstaff car park, just a few metres from CERN's reception area (Building 33).   Just a few metres from the CERN Reception, the new Novae snack point welcomes visitors and CERNois. Opening hours Currently: Monday to Friday, 8 a.m. to 4 p.m. From September: Monday to Friday, 7:45 a.m. to 5 p.m.; Saturdays from 8 a.m. to 2 p.m. The snack bar selection includes breakfast, starting at 2.70 CHF, cold dishes from 5 CHF, and hot dishes from 6 CHF.   Novae has also installed a 24-hour-a-day food vending machine in the CERN hostel (Building 39) and in Building 13. You can buy pasta and cooked dishes for 6.50 CHF to 8 CHF. In addition, a groceries vending machine has been installed in the main building, just across from the news kiosk. Nearly 60 different items are available around the clock. Finally, Novae has introduced a new payment system in several buildings on the Meyrin site. It accepts credit ca...

  6. Transferência de imunidade passiva em cordeiros de corte manejados extensivamente em clima tropical

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    C.F. Turquino

    2011-03-01

    Full Text Available Aspectos relacionados à transferência de imunidade passiva (TIP foram estudados em 290 cordeiros recém-nascidos, cruzas Texel, manejados extensivamente em contato permanente com as suas mães, e criados em clima tropical. Amostras de sangue foram colhidas dos cordeiros uma única vez entre 24 e 36 horas de vida para obtenção do soro sanguíneo. Foram determinadas a atividade da gama glutamiltransferase e as concentrações de proteínas totais por refratometria e colorimetria, de albumina, alfa, beta e gamaglobulinas por eletroforese e de IgG estimada pela turvação pelo sulfato de zinco. Os cordeiros foram agrupados de acordo com o sexo, o número de partos das ovelhas, o escore de condição corporal (ECC da ovelha, o número de cordeiros nascidos, o peso e a vitalidade ao nascimento. Os fatores de risco para a ocorrência de falha na transferência de imunidade passiva (FTIP foram identificados e a sua associação com a mortalidade de cordeiros foi testada. Foram estabelecidas correlações entre as variáveis estudadas. A TIP não foi influenciada pelo sexo, pelo número de partos ou pelo ECC das ovelhas. Houve diferenças entre os cordeiros únicos e gêmeos e entre os que nasceram com peso >3 kg e < 3 kg. A FTIP foi pouco frequente (12,4%, mais provável em gêmeos (p=0,026 e em cordeiros leves (p<0,001 e esteve fortemente associada com a mortalidade dos cordeiros até os 60 dias de vida (p<0,001. A taxa de mortalidade geral foi de 11,3%; e 30,5% dos cordeiros com FTIP morreram, quase todos no primeiro mês de vida. A concentração de proteína total determinada por refratometria se correlacionou (p<0,001 com as concentrações de gamaglobulinas (r=0,816 e de IgG (r=0,810 e o valor crítico < 5,0g/dL para a proteína total pode ser admitido como indicador de FTIP. Sob condições de clima tropical a FTIP pode ser considerada pouco frequente em cordeiros mestiços de corte, entretanto, a vigilância e os cuidados devem ser

  7. Magnetic novae

    Science.gov (United States)

    Zemko, Polina; Orio, Marina

    2016-07-01

    We present the results of optical and X-ray observations of two quiescent novae, V2491 Cyg and V4743 Sgr. Our observations suggest the intriguing possibility of localization of hydrogen burning in magnetic novae, in which accretion is streamed to the polar caps. V2491 Cyg was observed with Suzaku more than 2 years after the outburst and V4743 Sgr was observed with XMM Newton 2 and 3.5 years after maximum. In the framework of a monitoring program of novae previously observed as super soft X-ray sources we also obtained optical spectra of V4743 Sgr with the SALT telescope 11.5 years after the eruption and of V2491 Cyg with the 6m Big Azimutal Telescope 4 and 7 years post-outburst. In order to confirm the possible white dwarf spin period of V2491 Cyg measured in the Suzaku observations we obtained photometric data using the 90cm WIYN telescope at Kitt Peak and the 1.2 m telescope in Crimea. We found that V4743 Sgr is an intermediate polar (IP) and V2491 Cyg is a strong IP candidate. Both novae show modulation of their X-ray light curves and have X-ray spectra typical of IPs. The Suzaku and XMM Newton exposures revealed that the spectra of both novae have a very soft blackbody-like component with a temperature close to that of the hydrogen burning white dwarfs in their SSS phases, but with flux by at least two orders of magnitude lower, implying a possible shrinking of emitting regions in the thin atmosphere that is heated by nuclear burning underneath it. In quiescent IPs, independently of the burning, an ultrasoft X-ray flux component originates at times in the polar regions irradiated by the accretion column, but the soft component of V4743 Sgr disappeared in 2006, indicating that the origin may be different from accretion. We suggest it may have been due to an atmospheric temperature gradient on the white dwarf surface, or to continuing localized thermonuclear burning at the bottom of the envelope, before complete turn-off. The optical spectra of V2491 Cyg and V

  8. Desempenho de cordeiros alimentados com diferentes níveis protéicos

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    Zundt Marilice

    2002-01-01

    Full Text Available O experimento foi conduzido com o objetivo de avaliar níveis crescentes de proteína bruta (PB na dieta de cordeiros em confinamento, por meio de seus efeitos sobre o desempenho animal. Trinta e dois cordeiros "tricross" (¹/2 Texel + fraction one-quarter Bergamácia + fraction one-quarter Corriedale, sendo 16 machos inteiros e 16 fêmeas, com idade média de 5 meses e peso vivo de 30 kg , foram alimentados durante 57 dias com dietas isoenergéticas (72% NDT, variando os níveis protéicos (12, 16, 20 e 24 % PB. Os animais foram identificados, pesados e distribuídos nos quatro tratamentos. Os cordeiros permaneceram em baias individuais, cobertas, com piso ripado e suspenso. Os parâmetros estudados foram ganho de peso, consumo de matéria seca, conversão alimentar e o custo de produção do quilograma de carcaça. A utilização de dietas, com diferentes níveis protéicos na terminação de cordeiros, mostrou efeito linear positivo para ganho de peso e negativo para conversão alimentar. Verificou-se que a utilização de dietas com níveis protéicos crescentes não influenciou o consumo de matéria seca dos cordeiros. Observou-se viabilidade econômica na terminação de cordeiros, utilizando-se dietas entre 12 e 24% de PB, entretanto, o maior retorno foi obtido com a ração contendo 12% PB. Não houve efeito de sexo para os parâmetros analisados.

  9. INCA-MORENA, UNA NUEVA VARIEDAD DE PAPA DE PIEL MORADA PARA CONSUMO FRESCO

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    Juan G. Castillo Hernández

    2015-01-01

    Full Text Available El programa de mejoramiento genético de la papa(Solanum tuberosumL. en Cuba permite la selección de nuevasvariedades con características adecuadas a las exigencias actualesdel mercado y los cambios que originan las variaciones del clima.La obtención de la nueva variedad comenzó en la campaña 2005-2006, mediante el método tradicional de hibridación-selecciónde dos clones cubanos (14-52-93x11-18-96. Esta variedad sedistingue del resto de las obtenidas en el país en el color morado desu piel y la longitud del tallo, por encima de 70 cm. Se obtiene porprimera vez en el país una variedad con tubérculos de piel morada,buen comportamiento para el consumo fresco, alto potencial derendimiento y tolerancia en campo a la sarna común (Streptomicesscabies y al tizón temprano (Alternaria solani.

  10. Effect of the Purple Corn Beverage "Chicha Morada" in Composite Resin during Dental Bleaching.

    Science.gov (United States)

    Acuña, Eric Dario; Delgado-Cotrina, Leyla; Rumiche, Francisco Aurelio; Tay, Lidia Yileng

    2016-01-01

    During dental bleaching the staining potential of the surface would increase. This study aims to evaluate the staining susceptibility of one bleached composite resin after the exposure to three different beverages: Peruvian purple corn based beverage (chicha morada), green tea, and distilled water. Thirty disk-shaped specimens of one nanofill composite resin were prepared. The specimens were then divided into six groups (n = 5): purple corn (P), purple corn + bleaching (PB), green tea (T), green tea + bleaching (TB), distilled water (W), and distilled water + bleaching (WB). In groups that received bleaching, two sessions of bleaching with 35% hydrogen peroxide were done. Following bleaching, specimens were exposed to each liquid thirty minutes daily. Color was measured with a digital spectrophotometer. For statistical analysis, color measurement differences between the obtained results were used: during bleaching, after bleaching, and during + after bleaching. Two-way ANOVA was used to compare the color changes in the resins of all groups (p composite resin regardless of the bleaching procedure. However, purple corn was the only beverage that caused a perceptible color change (ΔE > 3.3).

  11. Pequeno surto de leishmaniose tegumentar americana em Macuco (Cordeiro - RJ

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    Jacqueline A. Menezes

    1974-06-01

    Full Text Available Por ocasião de um pequeno surto de leishmaniose tegumentar americana em localidade do município de Cordeiro (RJ foram documentados 14 casos. Entre os fatos que chamaram a atenção dos autores estão a alta ocorrência em crianças (57%, a freqüência do componente linfangítico (40%, a tendência à cicatrização espontânea e a distribuição peri-domiciliar dos casos. Um inquérito pela intradermoreação de Montenegro na área de maior concentração de casos, realizado numa fazendo e numa escola, mostrou 17% de reações positivas, 17% de duvidosas e 66% de reações negativas, num total de 117 indivíduos testados. Não foram encontrados casos antigos cicatrizados, o que sugere um foco recente. Discute-se o significado das reações duvidosas.

  12. MARCADORES MOLECULARES ASOCIADOS CON RESISTENCIA A LA ENFERMEDAD PUNTA MORADA EN PAPA

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    Ferm\\u00EDn Orona-Castro

    2009-01-01

    Full Text Available El objetivo de este trabajo fue identificar marcadores DNA Polimórfico Amplificado al Azar (RAPDs y Secuencias Simples Repetidas (SSR s también conocidos como Mi crosatélites asocia dos con la resistencia al daño causado por fitoplasmas en papa. Se evaluó la severidad de la punta morada de la papa (PMP y la apa rición de color pardo en el tubérculo, así como también se realizaron análisis moleculares en varie dades y líneas avanzadas de papa . El estudio se realizó en el laboratorio de biotecnología de la Facultad de Cie ncia s Biológicas de la Universidad Autónoma de Nuevo León - Instituto Na cional de Investigaciones Forestales Agrícolas y Pecuarias (INI FAP, México en el 2003 y 2004. Las técnicas utilizadas fueron RAPDs y SSRs también conocido microsatélites. Tres genotip os mostraron resistencia a la apa rición del color pardo deltubérculo, mie ntras que del análisis molecular seis materia les formaron un grupo que incluyó los genotip os con valores de daño mínimos (entre uno y tres de la escala. Los genotip os restantes formaron dos grupos con presencia de color pardo en el tubérculo mayor (entre cinco y siete. Se identificaron marcadores moleculares posiblemente asocia dos con tolerancia a la coloración parda del tubérculo. En el análisis de componentes principa les y el dendograma generado los materia les que presentaron menor severidad de daño, quedaron incluidos en un mismo grupo, mie ntras que materia les con mayor severidad de daño quedaron en un grupo diferente

  13. Efeitos da corticoterapia materna nos valores hemogasométricos de cordeiros nascidos a termo e prematuros

    Directory of Open Access Journals (Sweden)

    Francisco Leydson Formiga Feitosa

    Full Text Available RESUMO: O objetivo do estudo foi avaliar as variáveis hemogasométricas de cordeiros nascidos a termo e prematuros do nascimento às 48 horas de vida. Foram constituídos quatros grupos experimentais: PN (cordeiros nascidos de parto normal, n=15, média de 146 dias de gestação; PNDEX (cordeiros nascidos de parto normal, cujas mães receberam 16 mg de dexametasona aos 141 de gestação, n=8, média de 143 dias de gestação; PRE (cordeiros prematuros nascidos de cesarianas aos 138 dias de gestação, n=10 e PREDEX (cordeiros prematuros nascidos de cesarianas aos 138 dias de gestação, cujas mães receberam 16 mg de dexametasona dois dias antes do parto, n=9. Imediatamente após o nascimento, os cordeiros de todos os grupos apresentaram quadro de acidose respiratória (pH baixo e pCO2 elevada, com maior ênfase nos animais prematuros. A concentração de HCO3 - diminuiu entre 15 e 60 minutos de vida, principalmente nos grupos PRE e PREDEX, com posterior aumento no M24h. Os valores de diferença de base foram menores nos cordeiros prematuros, os quais apresentaram respiração abdominal, intensa dispneia e grande quantidade de líquido pulmonar. A estabilização do equilíbrio ácidobase ocorreu em todos os animais ao longo das primeiras 24 horas de vida. A dexametasona teve influência positiva sobre a condição clínica dos animais prematuros, resultando em adequada ventilação e perfusão tecidual, o que garantiu maior taxa de sobrevivência.

  14. Duas fontes de proteína na dieta de cordeiros confinados

    OpenAIRE

    Gallo, Sarita Bonagurio; MERLIN,Fernanda de Almeida; MACEDO,Cássio Moreira de; Reis, Viviane Aparecida Amin

    2015-01-01

    Objetivou-se comparar dietas para cordeiros em confinamento com dois níveis de proteína e duas fontes proteicas. Foram confinados 30 cordeiros machos, não-castrados, meio sangue Dorper com Santa Inês, com idade aproximada de 2,5 meses e peso vivo inicial médio de 23kg, divididos aleatoriamente em três tratamentos: dieta controle (15% PB), dieta com alta concentração de proteína verdadeira (farelo de soja, com 19% PB) e dieta com alta concentração de nitrogênio não protéico (uréia, 19% PB). O ...

  15. Chacal ou Cordeiro? O Brasil frente aos desafios e oportunidades do Sistema Internacional

    Directory of Open Access Journals (Sweden)

    Júlio César Cossio Rodriguez

    2012-12-01

    Full Text Available Este artigo analisa as configurações da política externa brasileira pós-2002 para relacionar os ganhos e perdas com as mudanças estruturais do sistema internacional. O intuito e realizar um balanço das capacidades materiais do Brasil, assim como dos seus desafios e oportunidades, a partir das categorias propostas por Randall Schweller. Chacal ou Cordeiro? Como se comporta o Brasil num sistema internacional em transição e quais podem ser as consequências? Ou seja, atua como chacal na busca de ganhos relativos ao seguir o ator mais revisionista (China, e como cordeiro na associação direta com a potência unipolar.

  16. Recovery of old novae

    Directory of Open Access Journals (Sweden)

    L. Schmidtobreick

    2004-01-01

    Full Text Available Durante un proyecto a largo plazo dedicado a la investigaci on de novas cl asicas con explosiones de grandes amplitudes hemos llevado a cabo fotometr a a m ultiples longitudes de onda y espectroscop a optica de varios candidatos de novas viejas. Introducimos aqu el objetivo del proyecto, la b usqueda de novas con baja trans- ferencia de masa y per odos orbitales cortos, y explicamos el m etodo para recuperar estas novas viejas a trav es de sus caracter sticas de color. Finalmente nos concentramos en los primeros resultados para una selecci on de objetos de nuestra muestra.

  17. Reatividade e desempenho em cordeiros cruzados Suffolk x Île-de-France

    Directory of Open Access Journals (Sweden)

    Priscilla Regina Tamioso

    2014-12-01

    Full Text Available Objetivou-se estimar as correlações fenotípicas (r entre os escores comportamentais de reatividade aplicados durante e após a pesagem e os ganhos médios diários de peso (GMD de cordeiros cruzados Suffolk x Île-de-France, aos 30, 60 e 90 dias de idade, bem como estudar o efeito da habituação dos animais ao manejo. As variáveis avaliadas por meio de escores foram: interferência do avaliador para o animal entrar na balança (INT, vocalização (VOC, movimentação (MOV, tensão (TEN, movimentos exploratórios (ME, postura de orelhas (ORE e o teste de tipos de marcha (TM. Os resultados das correlações de Spearman obtidos entre os escores indicam que VOC, MOV e TEN podem ser consideradas como características importantes na expressão da reatividade de ovinos em ambiente de restrição. Já o GMD parece não estar associado com a reatividade dos cordeiros avaliados. Por fim, aos 90 dias de idade, os cordeiros apresentaram-se menos reativos, em função do aprendizado por habituação

  18. Leishmaniose tegumentar canina em Morada das Águias (Serra da Tiririca, Maricá, Rio de Janeiro, Brasil

    Directory of Open Access Journals (Sweden)

    Cathia M. B. Serra

    2003-12-01

    Full Text Available Descreve-se a ocorrência da leishmaniose tegumentar em cães da localidade de Morada das Águias (Serra da Tiririca, Maricá, Estado do Rio de Janeiro, Brasil. Foram avaliados 83 cães por meio de exames clínico, sorológico e parasitológico. Os soros de 11 (13,2% animais foram reagentes à imunofluorescência indireta (IFI e de 30 (36,1% ao ensaio imunoenzimático (ELISA. Úlceras cutâneas e ou mucosas foram observadas em 18 (n = 83; 21,7% dos animais. Leishmania foi isolada de 11 cães. Discute-se a ocorrência da doença e a ocupação da localidade.

  19. Do berço ao berçário: a instituição como morada e lugar de contato

    Directory of Open Access Journals (Sweden)

    Marta Nörnberg

    2013-12-01

    Full Text Available Este ensaio aborda o sentido da instituição infantil a partir de uma perspectiva ético-estético-afetiva do viver humano. A abordagem ampara-se em perspectivas filosóficas sobre a existência humana. Os argumentos apresentam o berçário como morada, lugar do viver juntos, instituição que se faz em coletividade, nela e com ela, decorrente do encontro de bebês e adultos. Ao constituir-se como morada dos bebês, o berçário ritualiza e reatualiza a prática pedagógica como lugar de relação entre bebês e adultos, requerendo uma pedagogia do contato.

  20. Radioactive Nova Zembla; Nova Zembla radioactief

    Energy Technology Data Exchange (ETDEWEB)

    Duursma, E.

    1996-10-01

    The former Soviet Union dumped radioactive wastes in the seas around the island Nova Zembla (Novaya Zemlya) for decades. Complete nuclear reactors were sunk down. In this non-specialist article the risks from this Cold War heritage are discussed. 4 figs., 1 tab., 1 ref.

  1. Aplicação materna de glicocorticoide nos parâmetros vitais de cordeiros nascidos a termo e prematuros

    Directory of Open Access Journals (Sweden)

    Larissa Gabriela Avila

    2014-06-01

    Full Text Available O objetivo deste trabalho foi avaliar a influência do glicocorticoide sobre parâmetros vitais de cordeiros nascidos a termo e prematuros, do nascimento às 48 horas de vida. Foram constituídos quatros grupos: PN (cordeiros nascidos de parto normal, n=15, média de 146 dias; PNDEX (cordeiros nascidos de parto normal, cujas mães receberam 16mg de dexametasona aos 141 dias de gestação, n=8, média de 143 dias; PRE (cordeiros prematuros nascidos de cesarianas aos 138 dias de gestação, n=10; e PREDEX (cordeiros prematuros nascidos de cesarianas aos 138 dias de gestação, cujas mães receberam 16mg de dexametasona dois dias antes, n=9. As frequências cardíaca e respiratória variaram ao longo do período, com os maiores valores nos grupos de partos normais. A temperatura retal diminuiu em todos os grupos nos primeiros 60 minutos de vida, sendo os menores valores observados nos cordeiros prematuros, e o escore Apgar foi mais alto nos animais nascidos em tempo gestacional normal. Os cordeiros prematuros apresentaram menor vitalidade e menor taxa de sobrevivência, entretanto, menor taxa de mortalidade foi observada nos prematuros sob influência da dexametasona.

  2. Recurrent Novae - A Review

    CERN Document Server

    Mukai, Koji

    2014-01-01

    In recent years, recurrent nova eruptions are often observed very intensely in wide range of wavelengths from radio to optical to X-rays. Here I present selected highlights from recent multi-wavelength observations. The enigma of T Pyx is at the heart of this paper. While our current understanding of CV and symbiotic star evolution can explain why certain subset of recurrent novae have high accretion rate, that of T Pyx must be greatly elevated compared to the evolutionary mean. At the same time, we have extensive data to be able to estimate how the nova envelope was ejected in T Pyx, and it turns to be a rather complex tale. One suspects that envelope ejection in recurrent and classical novae in general is more complicated than the textbook descriptions. At the end of the review, I will speculate that these two may be connected.

  3. Waldemar Cordeiro: precursor of the tecno-poetic images in Brazil Waldemar Cordeiro: precursor das imagens tecno-poéticas no Brasil

    Directory of Open Access Journals (Sweden)

    Eduardo Ewald Maya

    2010-03-01

    Full Text Available This article presents the path of artist Waldemar Cordeiroconsidering his avant-garde trajectory, highlighting three importantmoments that accent his work: the painting – by expressionism,cubism, concrete and pop-art with the ready-mades -; the creation ofartistic objects with fragmented images newspapers, and, finally, theuse of computer to create new meanings with photography scanned. Este artigo apresenta o percurso do artista plásticoWaldemar Cordeiro, a partir da sua trajetória vanguardista,destacando três momentos importantes que marcaram a sua obra: apintura – pelo expressionismo, cubismo, concretismo e a pop-artecom os ready-mades - : a criação dos objetos artísticos com imagensfragmentadas de jornais; e por último, a utilização do computadorpara a criação de novos sentidos com a fotografia digitalizada.

  4. Nova Aquila 1919: a nova after all?

    CERN Document Server

    Lau, Herbert H B; Liu, X W

    2010-01-01

    Nova 1919 Aquila is today widely assumed to have been the result of a final helium shell flash occurring on a single post-asymptotic giant branch star. The fact that the outbursting star is in the middle of an old planetary nebula and that the ejecta associated with the outburst is hydrogen deficient supports this diagnosis. However, the material ejected during that outburst is also extremely neon rich, suggesting that it derives from an oxygen-neon-magnesium star, as is the case in the so-called neon novae. We have therefore attempted to construct a scenario that explains all the observations of the nebula and its central star, including the ejecta abundances. We find two scenarios that have the potential to explain the observations, although neither is a perfect match. The first scenario invokes the merger of a main sequence star and a massive oxygen-neon-magnesium white dwarf. The second invokes an oxygen-neon-magnesium classical nova that takes place shortly after a final helium shell flash. The main draw...

  5. OS EFEITOS DA URBANIZAÇÃO NO MICROCLIMA NO BAIRRO MORADA DA SERRA, CUIABÁ – MT

    Directory of Open Access Journals (Sweden)

    Laura Cristina da Silva VASCONCELOS

    2011-11-01

    Full Text Available Os efeitos da urbanização no ambiente geram uma atmosfera local com características climáticas próprias. Assim o objetivo foi analisar o microclima do bairro Morada da Serra, em Cuiabá-MT. Para tanto aplicou-se a metodologia do transecto móvel, coletando dados referentes à temperatura do ar e à nebulosidade às 20h, entre os dias 10 a 16/02/2008 (estação chuvosa e de 27/07 a 02/08/2008 (estação seca. Recorreu-se também ao índice pluviométrico, além da análise da variação das condições atmosféricas. Quanto a densidade de construções, a temperatura mais alta fixou-se no ponto com ocupação do espaço mais intensa, e a temperatura mais baixa situou-se no ponto localizado sobre um córrego margeado por mata ciliar e onde essa ocupação é rarefeita. Logo, é essencial um planejamento do espaço urbano que apresente soluções para se viver bem num ambiente saudável.

  6. Modos de vida alternativos: o caso da comunidade Noiva do Cordeiro

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    Adilson Schultz

    2011-04-01

    Full Text Available Noiva do cordeiro é uma comunidade rural liderada por mulheres, que desenvolveu um modo de vida alternativo e sustentável, com partilha de bens e fim da religião institucionalizada. Forjado ao longo de mais de um século, num processo de constantes rupturas religiosas, familiares e ideológicas, esse inusitado modo de vida produziu uma comunidade autônoma, com sujeitos autônomos e responsáveis uns pelos outros, que se tornaram lideranças sociais e políticas. No centro de sua história, experiências de sofrimento e rupturas relacionadas à religião, à fome, e à estrutura familiar patriarcal. O estudo do caso de Noiva do Cordeiro tem a intenção de analisar elementos subjetivos deste processo, verificando os indicativos e as implicações de tal fenômeno religioso e social, especialmente os limites e o fim de determinado modelo de religião. Os pressupostos teóricos deste estudo apontam para uma perspectiva transdisciplinar que compreende a teologia, a sociologia e a psicologia da religião e, nestes campos, as teorias feministas.

  7. Comportamento respiratório e qualidade pós-colheita de graviola (Annona muricata L. 'morada' sob temperatura ambiente Respiratory behavior and postharvest quality of 'morada' soursop (Annona muricata L. at room temperature

    Directory of Open Access Journals (Sweden)

    Maria Auxiliadora Coêlho de Lima

    2003-04-01

    Full Text Available Objetivou-se avaliar alterações físicas e físico-químicas, relacionando-as às taxas respiratória e de liberação de etileno, durante a maturação da graviola-'Morada'. Frutos colhidos na maturidade fisiológica foram armazenados (23,4 ± 1,1ºC e 81,8 ± 10,6% UR e avaliados aos 0; 1; 2; 3; 4 e 6 dias, quanto a: atividade respiratória (RS, liberação de etileno (ET, perda de matéria fresca, cor da casca e da polpa, firmeza, pH, acidez total titulável (ATT, sólidos solúveis totais (SST e açúcares solúveis totais (AST. Utilizou-se o delineamento experimental inteiramente casualizado, com quatro repetições. Aos dois dias, iniciou-se rápido aumento na RS, resultando no primeiro pico (197,60mg CO2·kg-1·h-1, que foi seguido por queda e uma fase lag. Ao término desta, iniciou-se o aumento climatérico (pico = 298,82mg CO2·kg-1·h-1. ET só foi detectada por ocasião do primeiro pico respiratório, atingindo o máximo aos quatro dias. A cor da casca tornou-se mais clara, enquanto na polpa se observou apenas redução da luminosidade. Houve coincidência entre o primeiro aumento na RS, o pico de ET e as mudanças mais significativas na firmeza, na ATT e nos teores de SST e AST. Durante o período, a firmeza diminuiu de 60 para 0,9N, e a ATT aumentou de 0,18 para 0,88% de ácido cítrico.It was aimed to evaluate physical and physico-chemical changes during soursop 'Morada' maturation at room temperature and related them to respiration rate and ethylene production. Fruits harvested at physiological maturity were stored (23,4 ± 1,1ºC and 81,8 ± 10,6% RH and evaluated at 0, 1, 2, 3, 4, and 6 days, according to: respiration rate (RS, ethylene production (ET, fresh weight lost, skin and pulp color, firmness, pH, total titrable acidity (TTA, total soluble solids (TSS and total soluble sugars (TS. The experimental design was a completely randomized one with four replications. There was a fast increase in RS at two days that resulted

  8. Síndrome de la orina morada en bolsa en paciente anciana con suplementos nutricionales Purple urine bag syndrome in elderly woman with nutritional supplements

    OpenAIRE

    A.R. Domínguez Alegría; M. Vélez Díaz-Pallares; M.ª A. Moreno Cobo; F. Arrieta Blanco; T. Bermejo Vicedo

    2012-01-01

    El síndrome de la orina morada en bolsa es una entidad poco frecuente que afecta característicamente a mujeres de edad avanzada con sondaje vesical prolongado y debilitadas por enfermedades crónicas. La presencia de patología urológica previa, el encamamiento prolongado y el estreñimiento crónico son factores predisponentes. El color morado de la orina se debe a la presencia de elevadas concentraciones de bacterias con actividad indoxilsulfatasa/fosfatasa que se desarrollan en un ambiente alc...

  9. New Novae snack point

    CERN Multimedia

    2012-01-01

    Located next to the car park by the flag poles, a few metres from the Main CERN Reception (building 33), a new snack point catered by Novae will open to the public on Wednesday 8 August. More information will be available in the next issue of the Bulletin!

  10. Aprendizagens e novas tecnologias

    Directory of Open Access Journals (Sweden)

    Pedro Demo*

    2011-06-01

    Full Text Available Pretendo aqui, muito preliminarmente, reunir alguns argumentos favoráveis à multiplicidade de oportunidades de aprender que o aluno pode encontrar hoje em ambientes de aprendizagem mediados por novas tecnologias. Centro-me principalmente na desconstrução de algumas resistências pedagógicas (EVANS, 2001 ainda persistentes entre nós como “transmissão de conteúdos”; agarramento a uma única teoria; fixação na aula instrucionista; extirpação/endeusamento de processos avaliativos, etc. Procuro ver, em um vasto âmbito de ofertas teóricas, componentes atualmente ressaltados na discussão tecnológica em vigor, com o objetivo de indicar oportunidades de reconstrução muito aproveitável de autores e clássicos, uma vez que aprender bem não foi algo inventado pelas novas tecnologias; sempre existiu e os grandes pedagogos tiveram consciência disso, insinuando infinitas maneiras de aprender bem (DEMO, 2008. As novas tecnologias proporcionam oportunidades ainda mais ampliadas, em meio também a enormes riscos e desacertos. O que menos interessa aqui é incidir em panaceias tecnológicas, bem a gosto do consumismo neoliberal. Interessa, porém, explorar novas oportunidades de aprendizagem, bem mais centradas na atividade dos alunos, flexíveis, motivadoras e capazes de sustentar processos de autoria e autonomia.

  11. Mechanisms of Secrets and Secrecy in «El secretario confuso» by Jacinto Cordeiro

    Directory of Open Access Journals (Sweden)

    Mariela Insúa Cereceda

    2015-11-01

    Full Text Available This article studies the mechanism of secrets and secrecy in El secretario confuso (1634, comedy by Jacinto Cordeiro; he is a playwright that belongs to the group of lusitan authors that write in Spanish during the Dual Monarchy period (1580-1640. This work, that can be included in the secretario subtype of comedia palatina genre —based on the infatuation between a noble lady and her secretary— shows thematic and structural coincidences with the main comedies of this moda­lity —El perro del hortelano by Lope de Vega and El vergonzoso en palacio by Tirso de Molina—, but providing new variations to this corpus focussed on the communicational dynamics of remaining silent, concealing and declaring love between the different characters.

  12. Concentração de lactato sérico em ovelhas e cordeiros mestiços (1/2 Suffolk nascidos em eutocia

    Directory of Open Access Journals (Sweden)

    L.P. Silva

    2013-08-01

    Full Text Available O objetivo do estudo foi avaliar a concentração de lactato sanguíneo venoso em ovelhas e em cordeiros neonatos imediatamente após o parto eutócico. Foram utilizadas 14 ovelhas, sendo nove da raça Suffolk e quatro mestiças e 20 cordeiros neonatos sadios (machos e fêmeas. O efeito do sexo, da raça e do número de cordeiros por parto foi investigado, bem como a possível correlação entre a concentração de lactato materno e neonatal. Não houve diferença entre machos e fêmeas, em relação à raça (Suffolk e mestiços, contudo a concentração de lactato foi mais elevada em cordeiros gêmeos ou trigêmeos quando comparado a cordeiros uníparos. Houve correlação positiva entre a concentração materna e a neonatal, sendo que quanto maior a concentração de lactato materno, maior a concentração no cordeiro imediatamente após o parto eutócico. Os resultados do presente estudo fornecem um subsídio por meio do qual se podem comparar os níveis de lactato sanguíneo em cordeiros em estado crítico.

  13. The Galactic Nova Rate Revisited

    CERN Document Server

    Shafter, A W

    2016-01-01

    Despite its fundamental importance, a reliable estimate of the Galactic nova rate has remained elusive. Here, the overall Galactic nova rate is estimated by extrapolating the observed rate for novae reaching $m\\leq2$ to include the entire Galaxy using a two component disk plus bulge model for the distribution of stars in the Milky Way. The present analysis improves on previous work by considering important corrections for incompleteness in the observed rate of bright novae. Several models are considered to account for differences in the assumed properties of bulge and disk nova populations. The simplest models, which assume uniform properties between bulge and disk novae, predict Galactic nova rates between $\\sim$50 to as many as $\\sim$100 per year, depending on the assumed incompleteness at bright magnitudes. Models where the disk novae are assumed to be more luminous than bulge novae are explored, and predict nova rates up to 30% lower, in the range of $\\sim$35 to $\\sim$70 per year. An average of the most p...

  14. Desempenho de cordeiros confinados, alimentados com dietas à base de torta de girassol

    Directory of Open Access Journals (Sweden)

    Deivison Novaes Rodrigues

    2013-04-01

    Full Text Available O objetivo deste trabalho foi avaliar os efeitos da inclusão da torta de girassol na dieta de cordeiros em confinamento sobre o desempenho produtivo dos animais. Utilizaram-se 40 cordeiros sem raça definida, não castrados, com peso médio inicial de 20,17±2,66 kg, alimentados com 0, 7, 14, 21 e 28% de torta de girassol na dieta (base seca. O experimento foi conduzido em delineamento de blocos ao acaso. A inclusão de torta de girassol na dieta não alterou o consumo médio de matéria seca (883,58 g por dia, a conversão alimentar (4,40 e o consumo médio de água (2,59 L por dia. O aumento dos níveis de torta de girassol diminuiu linearmente o peso final, o ganho de peso total, o ganho de peso diário e a área de olho de lombo. O nível de inclusão de até 28% não afeta o consumo médio de matéria seca e de água, mas reduz o desempenho e a área de olho de lombo. Para obter o menor custo com a dieta, o nível de inclusão da torta de girassol pode atingir até 28% da matéria seca, quando o seu preço representar até 40% do preço da mistura entre milho e farelo de soja.

  15. Glicerina bruta associada à silagem de sorgo em dietas para cordeiros

    Directory of Open Access Journals (Sweden)

    C.A.A. Oliveira Filho

    2015-04-01

    Full Text Available Objetivou-se avaliar os níveis de glicerina bruta (GB, 0, 20, 40, 60 e 80g/kg de matéria seca (MS de silagem de sorgo sobre a cinética da fermentação, 0, 30, 60 e 90g/kg de MS de silagem sobre a cinética de degradação da fibra em detergente neutro (FDN, e os níveis 0, 17, 33, 55 e 70g/kg de MS de silagem sobre o consumo e a digestibilidade da MS, os compostos nutricionais e o balanço de nitrogênio em cordeiros. O volume e a taxa de degradação dos carboidratos não fibrosos (Vcnf e (Kdcnf, respectivamente, apresentaram comportamento quadrático, sendo estimado Vcnf máximo (126,62mL/g de MS e Kdcnf mínima (0,0782/h para inclusão de 54,85g e 58,75g GB/kg de MS, respectivamente. Já o tempo de colonização (L, apresentou um decréscimo linear de 0,013h para cada 10g de GB/kg de MS. Houve redução linear de 0,996% na degradação para fração B. Não houve efeito significativo da inclusão de GB sobre o consumo e a digestibilidade da MS, os compostos nutricionais e o balanço de nitrogênio. A utilização de GB entre 50 e 70g/kg de MS em dietas à base de silagem de sorgo pode ser fonte alternativa de energia para cordeiros.

  16. Vila Nova de Gaia

    OpenAIRE

    Almeida, Salvador de Pinho Ferreira de

    2012-01-01

    Tese de doutoramento em Geografia, no ramo de Geografia Física, apresentado à Faculdade de Letras da Universidade de Coimbra The Old Historic Centre of Vila Nova de Gaia is a real living document of the life conditions and construction techniques of ancestral generations representative of cultural values, namely historical, architectural, urbanistic or just emotional that cannot be lost by neglect or carelessness, as they constitute a collective memory. It is necessary to draw ...

  17. NOVAS TECNOLOGIAS NO ENVELHECIMENTO

    Directory of Open Access Journals (Sweden)

    Rosa Maria Farah

    2010-02-01

    Full Text Available O Programa de Estudos Pós-Graduados em Gerontologia/PUC-SP desenvolve pesquisas em diversificadas linhas algumas das quais têm em comum o acolhimento à questão das novas tecnologias no envelhecimento. São investigações de caráter interdisciplinar que envolvem docentes-pesquisadores, orientandos de mestrado e de iniciação científica. Na área da educação a distância, a PUC-SP inaugura um trabalho em que o idoso interessado em avançar em seus conhecimentos é recebido em um ambiente virtual de aprendizagem, em que pode participar de cursos avançados de aquisição de novas linguagens e de navegação na Internet, cujas consequências são o investimento em uma via mais digna para o envelhecer no sentido de esse idoso sentir-se um ser ligado aos novos tempos em que a interatividade digital traz-lhe possibilidades ilimitadas de contatos com o outro, com o mundo enfim. A pesquisa sobre a inclusão cibersocial do idoso mostra o que significa colocar o idoso em contato com a Internet, quando este recebe, por meio das redes sociais, ofertas de várias ordens, e equipamentos que contornam limitações de ordem física ou motora. Além disso, o registro digital da memória do idoso, de sua história e referências também podem constituir conteudos preciosos para pesquisas. A relação do idoso com a informática pode situá-lo como um ator, produtor e reprodutor no ciberespaço. Isso significa que as vantagens do uso do computador fazem o idoso ganhar novo sentido na vida, na medida em que pode assim preencher o vazio causado pelas perdas que lhe vão ocorrendo, possibilitando que ele redimensione seu olhar para o presente e futuro. Palavras-chave: o sujeito-idoso nas novas tecnologias; novas tecnologias e envelhecimento; o idoso na educação a distância; internet na velhice.

  18. Recurrent Novae in M31

    CERN Document Server

    Shafter, A W; Rector, T A; Schweizer, F; Hornoch, K; Orio, M; Pietsch, W; Darnley, M J; Williams, S C; Bode, M F; Bryan, J

    2014-01-01

    The reported positions of 964 suspected nova eruptions in M31 recorded through the end of calendar year 2013 have been compared in order to identify recurrent nova candidates. To pass the initial screen and qualify as a recurrent nova candidate two or more eruptions were required to be coincident within 0.1', although this criterion was relaxed to 0.15' for novae discovered on early photographic patrols. A total of 118 eruptions from 51 potential recurrent nova systems satisfied the screening criterion. To determine what fraction of these novae are indeed recurrent the original plates and published images of the relevant eruptions have been carefully compared. This procedure has resulted in the elimination of 27 of the 51 progenitor candidates (61 eruptions) from further consideration as recurrent novae, with another 8 systems (17 eruptions) deemed unlikely to be recurrent. Of the remaining 16 systems, 12 candidates (32 eruptions) were judged to be recurrent novae, with an additional 4 systems (8 eruptions) b...

  19. Franchising in Nova Scotia

    Energy Technology Data Exchange (ETDEWEB)

    Hoffman, G. [Nova Scotia Petroleum Directorate, Halifax, NS (Canada)

    1998-09-01

    Opportunities for the local distribution of natural gas in Nova Scotia were reviewed, with special emphasis on franchising. Franchising in Nova Scotia began in 1980, made possible by the passage of the Gas Utilities Act and the Pipeline Act which promised western Canadian natural gas to eastern Canada. However, proposals for franchisees to distribute natural gas in the province were abandoned as the hope for natural gas transmission service to the province faded. The plummeting of world oil prices by the mid-1980s was also a contributory factor. Discovery and development of natural gas facilities around Sable Island led to the September 1997 proclamation of the Gas Distribution Act, which also led to the revival of interest in franchising. The Act provides for the competitive marketing of natural gas as a commodity and the regulation of the gas delivery system under a franchise agreement. Competitive applications are expected early in 1998, with awards of franchises in late 1998. Construction and gas delivery services should begin operations late in 1999.

  20. Terra Nova update

    Energy Technology Data Exchange (ETDEWEB)

    Carrick, G. [Petro-Canada, Inc. (Canada)

    2002-07-01

    This power point presentation shows a location map of the offshore oil and gas fields found off the Grand Banks of Newfoundland. It depicts the proximity of the Terra Nova oil field to Hibernia, White Rose, and the Hebron/Ben Nevis oil fields. The progress of the Terra Nova project since 2001 is described along with the commissioning challenges regarding turret and moorings as well as its modules, underwater components, flow lines, offshore marine operation, well construction and offshore start up. The 2002 operations schedule is also presented, along with production performance, and drilling/completions performance. A chart depicting environment, health and safety (EHS) indicators show that the current focus is on achieving superior environmental performance, injury free and to achieve the EHS performance target in the leading/lagging indicator ratio. Other current issues include the achievement of stable gas compression and sustained production, and to test the full capacity of the FPSO up to 150,000 barrels per day. The drivers of the first quartile performance include unit lifting costs, operating costs, and production efficiency. Operating costs include maintenance, platform support, logistics, onshore support, and well work. The project signifies tremendous growth opportunities for the east coast offshore petroleum industry. tabs., figs.

  1. Nova Mus 2008 = QY Mus

    Science.gov (United States)

    Templeton, Matthew R.

    2008-10-01

    Nova Mus 2008 = QY Mus was discovered by William Liller, Vina del Mar, Chile, on 2008 September 28.998 UT at magnitude 8.6 (Tech Pan film + orange filter). The position is RA = 13h 16m 36.44s , Dec = -67d 36m 47.8s (from P. Nelson). This object was announced as a nova in IAU Circular 8990 (Daniel W.E. Green, editor). The nova classification was determined using low-resolution spectra by W. Liller indicating the presence of broad H-alpha lines at least 2300 angstroms wide. Several observers confirmed the nova and provided photometry. The position above was provided by Peter Nelson (Ellinbank, Vic., Aus.), and is averaged from four separate exposures (rms error approx. 0.4 arcseconds). The GCVS team have formally designated Nova Mus 2008 as QY MUS. Observations should be reported to the AAVSO International Database as QY MUS.

  2. Processamento do presunto "cook-in" de cordeiros Processing of cook-in ham of lambs

    Directory of Open Access Journals (Sweden)

    Eliane Mattos Monteiro

    1999-12-01

    Full Text Available Este trabalho teve por objetivo desenvolver tecnologia para produto curado (presunto "cook-in", com pernis de cordeiros cruza Texel x Corriedale em associação com tratamentos tecnológicos (massagem em "tumbler" e processo "cook-in". O estudo foi desenvolvido pela EMBRAPA/CPPSUL e Universidade Federal de Santa Maria, RS, Brasil. Após as análises da composição química, a carne foi injetada manualmente com 20 % de salmoura composta por água + gelo 79%, cloreto de sódio 7,52%, condimento para presunto 4,70%, fosfatos 1,97%, sais de cura 1,88%, sacarose 3,38% e glutamato monossódico 0,19 %. Os presuntos foram avaliados quanto à composição química (umidade, proteína, gordura, cinzas, pigmentos totais e pH, parâmetros sensoriais (cor, aroma, sabor, textura e aceitabilidade e rendimento. Uma das principais características dos presuntos obtidos com pernil de cordeiros cruza Texel x Corriedale foi o baixo conteúdo de gordura associado ao bom rendimento e à excelente aceitabilidade.The aim of this study was to develop technology for the curing lambs (cook-in hams which were manufactured from the legs of crossbred Texel x Corriedale lambs in association with technologic treatment (massaging in tumbler and cook-in process. The experiment was conducted at the EMBRAPA-CPPSUL/ UFSM, RS, Brazil. After the evaluation of the chemical composition, the meat was injected with it manually - 20 % of brine containing water 79%, salt 7.52%, curing salts 1.88%, sucrose 3.38%, ham condiments 4.70%, phosphate 1.97% and sodium glutamate 0.19%. The ham quality was evaluated by analysis of its chemical composition (moisture, protein, ash, fat, pH, sensory properties (color, aroma, texture, acceptability and yield. The main characteristics of lamb hams were low fat contents associated with excellent acceptability and good yield.

  3. Efectos de la chicha morada y café sobre el esmalte dental bovino blanqueado con peróxido de hidrógeno

    OpenAIRE

    Castillo-Ghiotto, Gisella; Facultad de Estomatología, Universidad Peruana Cayetano Heredia. Lima.; Delgado-Cotrina, Leyla; Facultad de Estomatología, Universidad Peruana Cayetano Heredia. Lima.; Evangelista-Alva, Alexis; Facultad de Estomatología, Universidad Peruana Cayetano Heredia. Lima.

    2014-01-01

    Objetivo: El propósito de este estudio in vitro fue evaluar la susceptibilidad del esmalte dental bovino expuesto a chicha morada y café después del blanqueamiento con peróxido de hidrógeno (PH) al 35% con y sin calcio. Material y métodos: Setenta y dos dientes de bovino fueron blanqueados con peróxido de hidrógeno al 35% con y sin calcio (Whiteness HP Blue® - FGM y Whiteness HP Maxx® - FGM, respectivamente) y se expusieron al café instantáneo, refresco de maíz morado artificial y saliva (con...

  4. RECURRENT NOVAE IN M31

    Energy Technology Data Exchange (ETDEWEB)

    Shafter, A. W. [Department of Astronomy, San Diego State University, San Diego, CA 92182 (United States); Henze, M. [European Space Astronomy Centre, P.O. Box 78, E-28692 Villanueva de la Cañada, Madrid (Spain); Rector, T. A. [Department of Physics and Astronomy, University of Alaska Anchorage, 3211 Providence Dr., Anchorage, AK 99508 (United States); Schweizer, F. [Carnegie Observatories, 813 Santa Barbara St., Pasadena, CA 91101 (United States); Hornoch, K. [Astronomical Institute, Academy of Sciences, CZ-251 65 Ondřejov (Czech Republic); Orio, M. [Astronomical Observatory of Padova (INAF), I-35122 Padova (Italy); Pietsch, W. [Max Planck Institute for Extraterrestrial Physics, P.O. Box 1312, Giessenbachstr., D-85741, Garching (Germany); Darnley, M. J.; Williams, S. C.; Bode, M. F. [Astrophysics Research Institute, Liverpool John Moores University, Liverpool L3 5RF (United Kingdom); Bryan, J., E-mail: aws@nova.sdsu.edu [McDonald Observatory, Austin, TX 78712 (United States)

    2015-02-01

    The reported positions of 964 suspected nova eruptions in M31 recorded through the end of calendar year 2013 have been compared in order to identify recurrent nova (RN) candidates. To pass the initial screen and qualify as a RN candidate, two or more eruptions were required to be coincident within 0.′1, although this criterion was relaxed to 0.′15 for novae discovered on early photographic patrols. A total of 118 eruptions from 51 potential RN systems satisfied the screening criterion. To determine what fraction of these novae are indeed recurrent, the original plates and published images of the relevant eruptions have been carefully compared. This procedure has resulted in the elimination of 27 of the 51 progenitor candidates (61 eruptions) from further consideration as RNe, with another 8 systems (17 eruptions) deemed unlikely to be recurrent. Of the remaining 16 systems, 12 candidates (32 eruptions) were judged to be RNe, with an additional 4 systems (8 eruptions) being possibly recurrent. It is estimated that ∼4% of the nova eruptions seen in M31 over the past century are associated with RNe. A Monte Carlo analysis shows that the discovery efficiency for RNe may be as low as 10% that for novae in general, suggesting that as many as one in three nova eruptions observed in M31 arise from progenitor systems having recurrence times ≲100 yr. For plausible system parameters, it appears unlikely that RNe can provide a significant channel for the production of Type Ia supernovae.

  5. Persistence and change of the peasantry. A critical approach to "La morada de la vida" from contemporary Marxism Persistencia y cambio del campesinado. Un abordaje crítico a "La morada de la vida" desde el marxismo contemporáneo

    Directory of Open Access Journals (Sweden)

    Carolina Diez

    2009-01-01

    Full Text Available This work aims to identify and contrast the theoretical and methodological strategies used by Beatrice M. Alasia de Heredia and Bronislaw Galeski, to study the economic unit of rural production. We take as reference two works of authors that we consider most relevant for studies of peasantry: "La morada de la vida. Trabajo familiar de pequeños productores del nordeste de Brasil" (2003 y "Sociología del campesinado" (1977 respectively. While both works belong to different disciplinary traditions, analyzing the economic unit of rural production they consider its persistence in the capitalist economic system.Este trabajo se propone identificar y contrastar las estrategias teórico-metodológicas utilizadas por Beatriz M. Alásia de Heredia y Bronislaw Galeski, en el estudio de la unidad económica de producción campesina. Tomamos como referencia dos obras de los autores que consideramos sumamente relevantes para los estudios de campesinado: "La morada de la vida. Trabajo familiar de pequeños productores del nordeste de Brasil" (2003 y "Sociología del campesinado" (1977 respectivamente. Si bien, ambas obras pertenecen a tradiciones disciplinares diferentes, al analizar la unidad económica de producción campesina, consideran su persistencia en el sistema económico capitalista.

  6. Olivier Chesneau's Work on Novae

    Science.gov (United States)

    Millour, F.; Lagadec, E.

    2015-12-01

    Olivier Chesneau founded a brand new field of observational astrophysics with his attempts to resolve the novae expanding fireball from the very first days of the explosion. With the images he could get, he showed that novae do indeed explode in an aspherical way, leading to a change of paradigm for the physics of these yet-poorly understood catastrophic systems. He also set the stage for a new way of estimating novae distances, by directly measuring the sky-size of the fireball and comparing it with spectroscopic scales, taking into account the tremendous effects of the fireball geometry.

  7. Olivier Chesneau's work on novae

    CERN Document Server

    Millour, Florentin

    2016-01-01

    Olivier Chesneau founded a brand new field of observational astrophysics with his attempts to resolve the novae expanding fireball from the very first days of the explosion. With the images he could get, he showed that novae do indeed explode in an aspherical way, leading to a change of paradigm for the physics of these yet-poorly understood catastrophic systems. He also set the stage for a new way of estimating novae distances, by directly measuring the sky-size of the fireball and comparing it with spectroscopic scales, taking into account the tremendous effects of the fireball geometry.

  8. Morada al Sur

    Directory of Open Access Journals (Sweden)

    Francisco Javier Zuluaga

    1968-10-01

    Full Text Available En estos días, casi sin transparencia, he vuelto mi meditación hacia un texto de poesía. En un estante de mi biblioteca, imperceptible como la luz que se cierne entre los árboles, permanecía como un callado interlocutor. Quise, nuevamente, releerlo con un propósito determinado. Su lectura, para mí, significaba un punto de referencia para la comparación con los nuevos trabajos poéticos.

  9. Aspects of Power in the bilogy Próspera y Adversa fortuna de Duarte Pacheco by Jacinto Cordeiro

    OpenAIRE

    2012-01-01

    Este trabajo estudia la temática del poder y la privanza en la bilogía Próspera y Adversa fortuna de Duarte Pacheco (1621) de Jacinto Cordeiro, dramaturgo perteneciente al grupo de autores portugueses que escriben en castellano en la época de la Monarquía Dual (1580-1640). Se analizan ambas comedias, con especial atención a la relación que Duarte Pacheco mantiene con las figuras que ostentan el rango de autoridad monárquica. Asimismo se valora el desarrollo dramático del protagonista en tanto...

  10. Consumo e desempenho de cordeiros e borregos alimentados com dietas de alto concentrado de milho ou sorgo

    Directory of Open Access Journals (Sweden)

    R.S. Venturini

    Full Text Available RESUMO Objetivou-se avaliar os consumos de matéria seca, nutrientes e desempenho na terminação de cordeiros e borregos submetidos a dietas de alto concentrado de grão de milho ou sorgo. Foram utilizados 32 animais, sendo 16 cordeiros (dente de leite e 16 borregos (dois dentes da raça Corriedale. As dietas eram constituídas de feno de aveia- branca (Avena sativa, grão de milho (Zea mays ou de sorgo (Sorghum bicolor (L. Moench, farelo de soja (Glycine Max, calcário calcítico, bicarbonato de sódio e monensina. Os cordeiros apresentaram superioridade (P≤0,05 quanto ao CMS (% do PV e g/kg PV0,75, ao CPB (kg/dia, % do PV e g/kg PV0,75, ao CEE (% do PV, ao CFDN e ao CFDA (% do PV e g/kg PV0,75, ao CNDT (% do PV, ao ganho de peso médio diário, à conformação in vivo e à conversão alimentar. Por outro lado, o CEE, o CCHT e o CCNE (kg/dia, o peso vivo inicial, o peso vivo final e o peso vivo ao abate foram superiores (P≤0,05 na categoria dos borregos. Em relação aos grãos avaliados, verificou-se maior (P≤0,05 CEE (kg/dia, % do PV e g/kg PV0,75 e menor (P≤0,05 CFDN (% do PV e CFDA (kg/dia, % do PV e g/kg PV0,75 para os animais alimentados com dieta de alto concentrado à base de grão de milho em relação àqueles alimentados com grão de sorgo. Os cordeiros apresentam consumos relativos superiores aos borregos, porém sua resposta zootécnica é maior. O uso de dietas de alto concentrado de sorgo ou de milho proporcionou resultados semelhantes.

  11. Recurrent Novae — A Review

    Directory of Open Access Journals (Sweden)

    K. Mukai

    2015-02-01

    Full Text Available In recent years, recurrent nova eruptions are often observed very intensely in wide range of wavelengths from radio to optical to X-rays. Here I present selected highlights from recent multi-wavelength observations. The enigma of T Pyx is at the heart of this paper. While our current understanding of CV and symbiotic star evolution can explain why certain subset of recurrent novae have high accretion rate, that of T Pyx must be greatly elevated compared to the evolutionary mean. At the same time, we have extensive data to be able to estimate how the nova envelope was ejected in T Pyx, and it turns to be a rather complex tale. One suspects that envelope ejection in recurrent and classical novae in general is more complicated than the textbook descriptions. At the end of the review, I will speculate that these two may be connected.

  12. Nova Delphini 2013: Backyard Analysis of a Classical Nova

    Science.gov (United States)

    Reid, Piper

    2014-01-01

    On August 14, 2013, Nova Delphini was discovered by Koichi Itagaki. This nova erupted to a maximum brightness of magnitude 4.4 by August 16, 2013. The extraordinary brightness of this event has allowed many amateur astronomers to have the chance to study it. More than 750 amateur astronomers have contributed to the AAVSO photometry database of Nova Delphini.1 The amount and quality of spectroscopic data gathered is unprecedented as well, as over 700 individual spectra have been collected so far in the ARAS database.2 A nova is a class of variable star that undergoes a cataclysmic eruption, which can be observed through a sudden increase in brightness that declines over a series of months or years. At the center of a nova is an accreting white dwarf star which is collecting hydrogen from its surroundings. The accreting mass causes a nuclear reaction on the surface of the white dwarf and as the pressure increases the reaction becomes super-critical and a thermonuclear runaway is ignited causing the brightness increase as well as triggering the ejection of a shell of material form the star. The stages of a classical nova outburst are outlined along with techniques available to amateur astronomers for study of these phenomena. The author’s equipment and software setup are detailed. Results obtained using a low resolution grating, Schmidt-cassegrain telescope and CCD camera that were acquired while Nova Delphini was in the “fireball stage” 3 and subsequent “iron curtain phase”3 are compared and discussed. Results obtained using a high resolution spectroscope, Schmidt-cassegrain telescope and CCD camera that were acquired during the “lifting of the iron curtain phase”3 are also presented. References 1. Turner, Rebecca. “AAVSO - Nova Del 2013” 20 Aug 2013 Web. 8 Sep 2013 2. Tessier, Francois. “ARAS Spectral Database - Nova-Del-2013” 22 Sep 2013 Web. 22 Sep 2013 3. Shore, Steven N. “Spectroscopy of Novae - A User’s Manual” arXiv:1211.3176 [astro

  13. Modelling nova populations in galaxies

    CERN Document Server

    Chen, Hai-Liang; Yungelson, L R; Gilfanov, M; Han, Zhanwen

    2016-01-01

    Theoretical modelling of the evolution of classical and recurrent novae plays an important role in studies of binary evolution, nucleosynthesis and accretion physics. However, from a theoretical perspective the observed statistical properties of novae remain poorly understood. In this paper, we have produced model populations of novae using a hybrid binary population synthesis approach for differing star formation histories (SFHs): a starburst case (elliptical-like galaxies), a constant star formation rate case (spiral-like galaxies) and a composite case (in line with the inferred SFH for M31). We found that the nova rate at 10\\;Gyr in an elliptical-like galaxy is $\\sim 10-20$ times smaller than a spiral-like galaxy with the same mass. The majority of novae in elliptical-like galaxies at the present epoch are characterized by low mass white dwarfs (WDs), long decay times, relatively faint absolute magnitudes and long recurrence periods. In contrast, the majority of novae in spiral-like galaxies at 10\\;Gyr hav...

  14. Uso de vermicomposto favorece o crescimento de mudas de gravioleira (Annona muricata L. 'Morada' associadas a fungos micorrízicos arbusculares Use of earthworm manure improves growth of soursop seedlings (Annona muricata L. 'Morada' associated with arbuscular mycorrhizal fungi

    Directory of Open Access Journals (Sweden)

    Danielle Karla Alves da Silva

    2008-09-01

    Full Text Available A gravioleira, cujos frutos apresentam elevado potencial para exportação, é de fácil adaptação ao Semi-Árido nordestino, e a sua produção, economicamente importante, vem sendo estimulada. O uso de adubos orgânicos associados à inoculação com fungos micorrízicos arbusculares (FMA pode ser útil na formação de mudas frutíferas, porém o efeito da adição de adubo na simbiose com gravioleira (Annona muricata L. 'Morada' não é conhecido. Foi investigado o efeito de FMA multiplicado em substrato com resíduo orgânico na formação de mudas de gravioleira mantidas em substratos com fertilizante. O delineamento foi inteiramente casualizado, em fatorial de 2×5: 2 substratos (solo sem ou com 10% de vermicomposto e cinco tratamentos de inoculação (Acaulospora longula Spain & Schenck e Gigaspora albida Schenck & Smith produzidos em substratos com ou sem resíduo orgânico e controle não inoculado, com quatro repetições. Após 102 dias, avaliou-se: massa seca da parte aérea e radicular, altura, diâmetro do caule, taxa de crescimento, produção de esporos de FMA e de glomalina, atividade enzimática do solo, respiração microbiana, colonização micorrízica total, arbuscular e hifálica. Em geral, a inoculação com FMA estimulou o crescimento, mas no tratamento adubado as mudas em simbiose com G. albida não foram beneficiadas pela associação. O uso de vermicomposto estimulou a colonização micorrízica, a respiração microbiana, a atividade enzimática e a produção de glomalina no solo, porém reduziu a esporulação de A. longula. A utilização de FMA e vermicomposto pode constituir alternativa na produção de mudas de gravioleira, pois reduziu à metade o tempo de formação das mudas e pode reduzir em 75% a dose de adubo a ser aplicada. No entanto, a escolha de FMA compatíveis com o hospedeiro é indispensável para garantir respostas positivas. A aplicação conjunta de FMA e adubo orgânico também pode

  15. Características da pastagem de azevém e produtividade de cordeiros em pastejo Ryegrass pasture characteristics and lamb productivity in grazing

    Directory of Open Access Journals (Sweden)

    Ticiany Maria Dias Ribeiro

    2009-03-01

    Full Text Available Objetivou-se avaliar a produção da pastagem de azevém, a qualidade da forragem e a produtividade animal por área em três sistemas de produção: cordeiros desmamados precocemente, aos 40 dias de idade, e mantidos em pastagem de azevém (Lolium multiflorum Lam. até o abate; cordeiros sem desmame, mantidos na mesma pastagem de azevém até o abate; cordeiros sem desmame recebendo suplemento (1% do peso vivo em creep feeding a partir dos 40 dias de idade. O sistema de pastejo utilizado foi o de lotação contínua com carga animal variável, mantendo-se a oferta de massa de lâminas foliares em 1.000 kg de MS/ha. A produção média de massa seca da pastagem foi 3.236,6 kg MS/ha, a de lâminas foliares, de 1.008,7 kg MS/ha, e a taxa de crescimento do pasto, de 58,38 kg MS/ha/dia. Com cordeiros desmamados, a altura média da pastagem foi de 20,95 cm, significativamente maior que a daquela com cordeiros sem desmame. A massa de inflorescências nas pastagens dos cordeiros desmamados foi superior (61,7 kg/ha quando comparado aos outros sistemas. O sistema de terminação de cordeiros desmamados permitiu maior carga animal (929,74 kg PV/ha em comparação aos demais, considerando apenas os cordeiros sem suplementação (259,9 kgPV/ha ou com suplementação em creep feeding (254,3 kgPV/ha. A qualidade da forragem não diferiu entre os sistemas de terminação. A estrutura da pastagem sofreu alterações na ausência das ovelhas, devido à maior seletividade dos cordeiros. O sistema de terminação em pastagem com desmame precoce foi o menos produtivo, em razão do baixo desempenho individual dos cordeiros, por isso, não deve ser recomendado a ovinocultores.The objective of this study was to evaluate the ryegrass pasture production, forage quality and animal productivity in three sheep production systems: lambs weaned at 40 days of age and finished in ryegrass (Lolium multiflorum Lam. until slaughter; lambs kept with their dams in the same pasture

  16. A nova ordem repressiva

    Directory of Open Access Journals (Sweden)

    Paulo Roberto Ceccarelli

    Full Text Available Segundo o autor, a humanidade sempre foi marcada por alguma forma de controle de acordo com o discurso do momento sociohistórico que atravessa: esse texto discute alguns instrumentos de controle e repressão da contemporaneidade. Se, por séculos, foi a religião que ditou as normas sociais, na modernidade, as verdades religiosas foram substituídas por enunciados científicos que sugeriam uma linearidade histórica e propunham uma compreensão determinista do mundo, baseada na capacidade da ciência em dar respostas. As certezas da modernidade foram radicalmente questionadas na pósmodernidade, fazendo surgir outros mecanismos de controle. Para o autor, a necessidade do ser humano de criar representações e dispositivos para suportar e nomear a angústia inerente ao desamparo que lhe é próprio o leva a submeter-se aos mais variados discursos repressivos. O discurso científico atual vem sendo transformado em instrumento ideológico que, com as inúmeras expressões do politicamente correto, traduzem uma busca de normatização e de padronização de comportamentos, gerando uma nova ordem repressiva. No que diz respeito à saúde psíquica, os manuais de diagnóstico, financiados pela indústria farmacêutica, transformam comportamentos, individualidades e diversidades em patologias: as singularidades tornam-se anormalidades. Qual é o compromisso social dos psicólogos nesse debate?

  17. Nova LMC 1990 no. 1: The first extragalactic neon nova

    Science.gov (United States)

    Sonneborn, George; Shore, Steven N.; Starrfield, Sumner G.

    1990-01-01

    International Ultraviolet Explorer (IUE) observations of nova LMC (Large Magellanic Cloud) 1990 No. 1, the first neon (or ONeMg) nova observed outside the Galaxy are presented. The observations were obtained from 17 Jan. to Mar. 1990, with especially dense coverage during the first 25 days of the outburst. (The neon nova categorization is based on the detection of forbidden Ne 3-4 lines in optical spectra; the ultraviolet neon lines were not detected.) During the first 30 days of the outburst, the radiative losses were dominated by the N 5 delta 1240 and C 4 delta 1550 lines. The maximum ejection velocity was approximately 8000 km/s, based on the blue absorption edge of the C 4 P-Cygni profile. Early in the outburst of Nova LMC 1990 No. 1 the UV luminosity alone was approximately 3 times 10 to the 38th power erg/sec, implying that the bolometric luminosity was well in excess of the Eddington luminosity for a one solar mass object.

  18. Síndrome de la orina morada en bolsa en paciente anciana con suplementos nutricionales Purple urine bag syndrome in elderly woman with nutritional supplements

    Directory of Open Access Journals (Sweden)

    A. R. Domínguez Alegría

    2012-12-01

    Full Text Available El síndrome de la orina morada en bolsa es una entidad poco frecuente que afecta característicamente a mujeres de edad avanzada con sondaje vesical prolongado y debilitadas por enfermedades crónicas. La presencia de patología urológica previa, el encamamiento prolongado y el estreñimiento crónico son factores predisponentes. El color morado de la orina se debe a la presencia de elevadas concentraciones de bacterias con actividad indoxilsulfatasa/fosfatasa que se desarrollan en un ambiente alcalino en presencia de otros factores. En el caso que presentamos la administración de suplementos nutricionales ricos en triptófano tuvieron un papel relevante en la generación de este síndrome.The purple urine bag syndrome is a rare entity which typically affects elderly women with prolonged urinary catheterization and weakening chronic diseases. Other predisposing factors are previous urologic pathology, immobility syndrome and chronic constipation. The purple color is due to the presence of high loads of bacteria with sulphatase - phosphatase activity which develop in an alkaline environment as well as the presence of other factors. In the case we present the administration of nutritional supplements containing tryptophan conditioned the generation of this syndrome.

  19. Níveis de energia no desempenho e características da carcaça de cordeiros alimentados em creep feeding

    Directory of Open Access Journals (Sweden)

    Garcia Cledson Augusto

    2003-01-01

    Full Text Available O trabalho foi realizado no Setor de Ovinocultura da Universidade de Marília, objetivando estudar os efeitos de três níveis de energia (2,6; 2,8 e 3,0 Mcal EM/kg MS na ração de cordeiros inteiros Suffolk criados em creep feeding, sobre o desempenho e características de carcaça. Na parição numerava-se e registravam-se o peso ao nascer dos cordeiros que, posteriormente, foram distribuídos aleatoriamente, compondo doze repetições por tratamento. As rações foram isoprotéicas (18,46% PB fornecidas ad libitum duas vezes ao dia, pesando-se as respectivas sobras. Os cordeiros foram pesados a cada 14 dias, permanecendo com as ovelhas até atingirem o peso vivo final, preestabelecido em 31 kg. Em seguida, os cordeiros permaneceram em jejum alimentar por 16 horas, até o momento do abate, obtendo-se o peso vivo ao abate. Após o abate, registraram-se os pesos da carcaça quente e do conteúdo digestivo, para o cálculo do peso de corpo vazio. As carcaças permanecerem por 24 horas na câmara de refrigeração em temperatura de 5ºC, obtendo-se o peso da carcaça fria. Para o ganho médio diário ocorreu diferença significativa entre os tratamentos, utilizando-se como covariável a idade de abate, com melhor desempenho para os cordeiros que receberam a ração com 3,0 Mcal EM. Para as características da carcaça não houve efeito dos tratamentos. Concluiu-se que o nível 3,0 Mcal EM foi o mais indicado para a ração de cordeiros Suffolk alimentados e terminados em creep feeding.

  20. Processamento do milho grão sobre desempenho e saúde ruminal de cordeiro

    Directory of Open Access Journals (Sweden)

    Letícia Silva Oliveira

    2015-07-01

    Full Text Available Vinte e dois cordeiros machos não castrados, Dorper x Santa Inês, com aproximadamente 90 dias de idade e peso vivo médio inicial de 27,0±4,4kg, foram alimentados com uma dieta com elevada proporção de concentrado com 20% de pelete proteico-mineral (Grano Entero(r, 5% de feno de capim coast-cross e 75% de milho, na forma de milho grão inteiro (MGI, milho grão moído (MGM ou milho grão úmido (MGU, para avaliação de desempenho no confinamento por um período de 14 dias de adaptação às dietas e às instalações e de 65 dias de confinamento. Em seguida, os animais foram abatidos com peso vivo médio final (PVF de 47,97±5,13kg e o conteúdo gástrico foi avaliado para quantificação de protozoários, e foi realizada avaliação papilar. O delineamento experimental foi o de blocos casualizados. Não houve diferença entre os tratamentos (P>0,05 quanto ao ganho de peso médio diário, eficiência alimentar, ingestão diária de matéria seca, características da carcaça e da carne. Os animais tratados com MGI tiveram maior conteúdo gástrico, menor pH ruminal, maior AP (% da superfície de absorção e maior área papilar em comparação com os outros tratamentos. Os animais tratados com MGI tiveram melhores resultados para o peso final, mas para os demais parametros estudados não foi observada diferença.

  1. Status for CASA NOVA konsortiet

    DEFF Research Database (Denmark)

    Bonke, Sten

    1997-01-01

    The report reviews the development projects and the results hitherto achieved by the design and build organisation CASA NOVA which is one of four consortia within the R&D programme "Process and Product Development in Building", financed by the Ministry of Industry and the Ministry of Housing....

  2. Status for CASA NOVA konsortiet

    DEFF Research Database (Denmark)

    Bonke, Sten

    1997-01-01

    The report reviews the development projects and the results hitherto achieved by the design and build organisation CASA NOVA which is one of four consortia within the R&D programme "Process and Product Development in Building", financed by the Ministry of Industry and the Ministry of Housing....

  3. Novae in gamma-rays

    CERN Document Server

    Hernanz, M

    2013-01-01

    Classical novae produce radioactive nuclei which are emitters of gamma-rays in the MeV range. Some examples are the lines at 478 and 1275 keV (from 7Be and 22Na) and the positron-electron annihilation emission (511 keV line and a continuum below this energy, with a cut-off at 20-30 keV). The analysis of gamma-ray spectra and light curves is a potential unique and powerful tool both to trace the corresponding isotopes and to give insights on the properties of the expanding envelope determining its transparency. Another possible origin of gamma-rays is the acceleration of particles up to very high energies, so that either neutral pions or inverse Compton processes produce gamma-rays of energies larger than 100 MeV. MeV photons during nova explosions have not been detected yet, although several attempts have been made in the last decades; on the other hand, GeV photons from novae have been detected in some particular novae, in symbiotic binaries, where the companion is a red giant with a wind, instead of a main ...

  4. Comportamento ingestivo de cordeiros em confinamento, alimentados com dieta exclusiva de concentrado com diferentes porcentagens de proteína

    Directory of Open Access Journals (Sweden)

    L.G.A. Cirne

    2014-02-01

    Full Text Available O experimento foi realizado com o objetivo de avaliar o comportamento ingestivo de cordeiros em confinamento, alimentados com dieta exclusiva de concentrado com diferentes porcentagens de proteína (14, 16, 18 e 20%. Foram utilizados 24 cordeiros mestiços da raça Santa Inês, não castrados, com aproximadamente 180 dias de idade, peso vivo médio de 25kg, confinados, num delineamento experimental inteiramente ao acaso, com quatro tratamentos e seis repetições. O tempo despendido na atividade de alimentação decresceu linearmente em 0,20 hora/dia para cada 1% de aumento na porcentagem de proteína na dieta; o de ócio aumentou linearmente em 0,25 hora/dia; e o de mastigação total reduziu linearmente em 0,25 hora/dia. A elevação da porcentagem de proteína na dieta elevou linearmente a eficiência de alimentação (kg MS e FDN/hora, em 0,038 e 0,005kg/hora, respectivamente, para as frações MS e FDN. Contudo, os consumos de matéria seca (MS e fibra em detergente neutro (FDN, a eficiência de ruminação (kg MS e FDN/hora, assim como o período (nº/dia e o tempo (min gasto por período de alimentação, ruminação e ócio não foram influenciados pelas diferentes porcentagens de proteína na dieta.

  5. AT Cnc: A SECOND DWARF NOVA WITH A CLASSICAL NOVA SHELL

    Energy Technology Data Exchange (ETDEWEB)

    Shara, Michael M.; Mizusawa, Trisha; Zurek, David [Department of Astrophysics, American Museum of Natural History, Central Park West at 79th Street, New York, NY 10024-5192 (United States); Wehinger, Peter [Steward Observatory, the University of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721 (United States); Martin, Christopher D.; Neill, James D.; Forster, Karl [Department of Physics, Math and Astronomy, California Institute of Technology, 1200 East California Boulevard, Mail Code 405-47, Pasadena, CA 91125 (United States); Seibert, Mark [Observatories of the Carnegie Institution of Washington, 813 Santa Barbara Street, Pasadena, CA 91101 (United States)

    2012-10-20

    We are systematically surveying all known and suspected Z Cam-type dwarf novae for classical nova shells. This survey is motivated by the discovery of the largest known classical nova shell, which surrounds the archetypal dwarf nova Z Camelopardalis. The Z Cam shell demonstrates that at least some dwarf novae must have undergone classical nova eruptions in the past, and that at least some classical novae become dwarf novae long after their nova thermonuclear outbursts, in accord with the hibernation scenario of cataclysmic binaries. Here we report the detection of a fragmented 'shell', 3 arcmin in diameter, surrounding the dwarf nova AT Cancri. This second discovery demonstrates that nova shells surrounding Z Cam-type dwarf novae cannot be very rare. The shell geometry is suggestive of bipolar, conical ejection seen nearly pole-on. A spectrum of the brightest AT Cnc shell knot is similar to that of the ejecta of the classical nova GK Per, and of Z Cam, dominated by [N II] emission. Galaxy Evolution Explorer FUV imagery reveals a similar-sized, FUV-emitting shell. We determine a distance of 460 pc to AT Cnc, and an upper limit to its ejecta mass of {approx}5 Multiplication-Sign 10{sup -5} M {sub Sun }, typical of classical novae.

  6. Identifying and Quantifying Recurrent Novae Masquerading as Classical Novae

    CERN Document Server

    Pagnotta, Ashley

    2014-01-01

    Recurrent novae (RNe) are cataclysmic variables with two or more nova eruptions within a century. Classical novae (CNe) are similar systems with only one such eruption. Many of the so-called 'CNe' are actually RNe for which only one eruption has been discovered. Since RNe are candidate Type Ia supernova progenitors, it is important to know whether there are enough in our galaxy to provide the supernova rate, and therefore to know how many RNe are masquerading as CNe. To quantify this, we collected all available information on the light curves and spectra of a Galactic, time-limited sample of 237 CNe and the 10 known RNe, as well as exhaustive discovery efficiency records. We recognize RNe as having (a) outburst amplitude smaller than 14.5 - 4.5 * log(t_3), (b) orbital period >0.6 days, (c) infrared colors of J-H > 0.7 mag and H-K > 0.1 mag, (d) FWHM of H-alpha > 2000 km/s, (e) high excitation lines, such as Fe X or He II near peak, (f) eruption light curves with a plateau, and (g) white dwarf mass greater tha...

  7. Avaliação da transferência de imunidade passiva em cordeiros com até 30 dias de idade

    Directory of Open Access Journals (Sweden)

    Flávia Corbari Féres

    2010-06-01

    Full Text Available O objetivo deste estudo foi determinar as concentrações séricas de imunoglobulina G, PT e de sua fração eletroforética γ globulina, assim como a atividade enzimática de GGT e ALP. Estabeleceu-se a possibilidade da atividade destas enzimas ser utilizada indiretamente como indicadoras de um adequado nível de proteção humoral e/ou como falha de transferência de imunidade passiva em cordeiros. Foi pesquisada a correlação entre as variáveis em quatro grupos de idade divididos em até 30 dias de vida. Para tanto, foram coletadas 191 amostras de sangue de cordeiros em 21 propriedades da região de Araçatuba - São Paulo. Realizaram-se os testes de imunodifusão radial, espectrofotometria e eletroforese para obtenção dos valores de IgG, PT e γ globulina, respectivamente. Para os valores da atividade de GGT e ALP, foram utilizados kits comerciais. Notou-se correlação significativa entre ALP e GGT, fato observado também com PT, IgG e GGT. A γ-globulina mostrou-se correlacionada com GGT, IgG e PT. A atividade de FA não deve ser utilizada como indicadora de transferência de imunidade passiva em cordeiros.

  8. AT Cnc: A Second Dwarf Nova with a Classical Nova Shell

    CERN Document Server

    Shara, Michael M; Wehinger, Peter; Zurek, David; Martin, Christopher D; Neill, James D; Forster, Karl; Seibert, Mark

    2012-01-01

    We are systematically surveying all known and suspected Z Cam-type dwarf novae for classical nova shells. This survey is motivated by the discovery of the largest known classical nova shell, which surrounds the archetypal dwarf nova Z Camelopardalis. The Z Cam shell demonstrates that at least some dwarf novae must have undergone classical nova eruptions in the past, and that at least some classical novae become dwarf novae long after their nova thermonuclear outbursts, in accord with the hibernation scenario of cataclysmic binaries. Here we report the detection of a fragmented "shell", 3 arcmin in diameter, surrounding the dwarf nova AT Cancri. This second discovery demonstrates that nova shells surrounding Z Cam-type dwarf novae cannot be very rare. The shell geometry is suggestive of bipolar, conical ejection seen nearly pole-on. A spectrum of the brightest AT Cnc shell knot is similar to that of the ejecta of the classical nova GK Per, and of Z Cam, dominated by [NII] emission. Galex FUV imagery reveals a ...

  9. Nova Scotia offshore renewal plan

    Energy Technology Data Exchange (ETDEWEB)

    NONE

    2008-10-15

    Increase in global exploration and production have caused a reduction in offshore exploration licences. This paper outlined the government of Nova Scotia's offshore renewal plan. The plan was designed to clarify the role of the government and the Canada-Nova Scotia Offshore Petroleum Board (CNSOPB) and federal government. The plan was comprised of 4 different sections, including (1) geoscience, (2) new policy, (3) regulation, and (4) investment abstraction. Requests for proposals are now being designed to develop a better understanding of the geology of offshore Nova Scotia, including the shelf slope and deep water areas in the vicinity of Sable Island. A code of practice is currently being developed to minimize the impact of resource development on the marine environment while supporting the economic development of smaller oil and gas discoveries. Resource and analysis packages are currently being developed to help investors compute the risks associated with developing offshore sites. It was concluded that early action is required to address challenges and knowledge gaps related to geological data, regulatory efficiency, policy, and marketing strategies. Success of the plan will require the continued cooperation, and support of various governmental agencies. Details of regulatory renewal initiative projects were included. 1 fig.

  10. Níveis de feno de alfafa e forma física da ração no desempenho de cordeiros em creep feeding

    Directory of Open Access Journals (Sweden)

    Neres Marcela Abbado

    2001-01-01

    Full Text Available Com o objetivo de avaliar o desempenho de cordeiros em creep feeding e confinados, foram realizados dois experimentos. No primeiro, 32 cordeiros ¾ mestiços Suffolk foram criados em creep feeding, desmamados aos 56 dias de idade e, em seguida, confinados. Os cordeiros receberam os seguintes tratamentos: 1. sem suplementação; 2. suplementação com ração à base de milho e soja; 3. ração à base de milho e soja com 15% de feno de alfafa; 4. ração à base de milho e soja com 30% de feno de alfafa. Após o desmame, os cordeiros suplementados foram confinados, recebendo a mesma ração do creep feeding até atingirem de 30 a 32 kg de peso vivo. No segundo experimento, foram utilizados 32 cordeiros ¾ mestiços Suffolk, alimentados em creep feeding, recebendo ração farelada ou peletizada até os pesos de abate: 26 e 28 kg. As dietas eram isoprotéicas (21% PB e isoenergéticas (2,9 Mcal EM/kg MS. Os animais suplementados na fase de aleitamento obtiveram ganho de peso de 147,4g/dia a mais, quando comparados aos não suplementados. Não houve efeito dos níveis de feno de alfafa na ração sobre o desempenho dos animais. Entretanto, no confinamento, a máxima eficiência de ganho de peso esperada para os machos, conforme a análise de regressão, situou-se em 18,7% de inclusão de feno de alfafa na ração. A ração peletizada propiciou maior desenvolvimento dos animais, quando comparada à ração farelada. Os machos que receberam ração peletizada atingiram os pesos de abate de 26 e 28 kg aos 55 e 60 dias de idade, respectivamente.

  11. Parâmetros hematológicos e perfil bioquímico renal de cordeiros nascidos a termo e prematuros

    Directory of Open Access Journals (Sweden)

    F.L. F. Feitosa

    Full Text Available RESUMO O objetivo do presente estudo foi avaliar as variáveis hematológicas e o perfil bioquímico renal sérico de cordeiros nascidos a termo e prematuros do nascimento às 48 horas de vida, bem como verificar a influência da dexametasona sobre tais variáveis. Foram constituídos quatros grupos experimentais: PN (cordeiros nascidos de parto normal, n=15, média de 146 dias; PNDEX (cordeiros nascidos de parto normal cujas mães receberam 16mg de dexametasona aos 141 de gestação, n=8, média de 143 dias; PRE (cordeiros prematuros nascidos de cesarianas aos 138 dias de gestação, n=10 e PREDEX (cordeiros prematuros nascidos de cesarianas aos 138 dias de gestação cujas mães receberam 16mg de dexametasona dois dias antes, n=9. Os valores médios do volume globular e de hemoglobina diminuíram ao longo das 48 horas de observação, nos quatro grupos experimentais, porém dentro dos limites fisiológicos para a espécie. Houve variação da concentração plasmática de proteínas totais em todos os momentos, sendo os menores valores no grupo PRE. A contagem leucocitária foi mais alta no grupo PN apenas no M24h. Ao longo do período, apenas o grupo PN mostrou diferença entre o M24h e os demais momentos, e o grupo PRE apresentou os menores valores de neutrófilos no M0h, M15min e M60min. As concentrações séricas de creatinina foram mais altas no grupo PRE no M60min, M24h e M48h. Em todos os grupos, houve diminuição no M24h e M48h. Os parâmetros avaliados foram afetados pela prematuridade na espécie ovina e a dexametasona teve influência positiva sobre a taxa de sobrevivência dos animais prematuros.

  12. Nutritional value of silk flower hay for lambs Valor nutritional do feno de flor-de-seda para cordeiros

    Directory of Open Access Journals (Sweden)

    Aderbal Marcos de Azevêdo Silva

    2010-12-01

    Full Text Available It was evaluated four levels of silk flower (Calotropis procera S.W. hay (SFH as a substitute of sorghum (Sorghum bicolor hay (SBH in diet for lambs. Nutritional value of silk-flower hay was determined based on aparent digestibility and on metabolic, productive and economical performance of Santa Inês lambs. It was used twenty-four castrated males at 15.72 ± 1.92 kg body weight randomly distributed in four diets with silk-fklower and sorghum hay ratios (100:0, 66:33, 33:66, 0:100, and supplemented with a concentrate mixture based on 50% roughage:50% concentrate (weight/weight. Increase in the levels of silk-flower hay in the diet reduced weight gain and nutrient intake and it increased feed conversion and digestibility coeficients of all the nutrients. Nitrogen balance was similar in all levels of silk-flower hay, although there was a tendency of reduction in nitrogen retention at levels 66% and 100% of silk-flower hay. At the levels 0 and 33% of silk-flower hay in the diet, dry matter ingestion (170 and 180 g/day, daily average weight gain (84 and 89 g/kg0.75and feed conversion (4.99 and 5.02 were satisfactory. Silk-flower hay can represent up to 16.5% of the total food ingestion or 33% of the roughage in diet for lambs.Avaliaram-se quatro níveis de feno de flor-de-seda (Calotropis procera S.W. em substituição ao feno de sorgo (Sorghum bicolor na dieta de cordeiros. O valor nutricional do feno de flor-de-seda foi determinado com base na digestibilidade aparente e no desempenho metabólico, produtivo e econômico de cordeiros Santa Inês. Utilizaram-se 24 machos castrados com peso corporal de 15,72 kg ± 1,92 kg distribuídos aleatoriamente em quatro dietas com relações entre feno de flor-de-seda e de sorgo (100:0, 66:33, 33:66 e 0:100 e suplementadas com uma mistura concentrada à base de 50% de volumos e 50% de concentrado (peso/peso. O aumento nos níveis de feno de flor-de-seda na dieta diminuiu o ganho de peso e a ingestão de

  13. Predicting a Luminous Red Nova

    Science.gov (United States)

    Van Noord, Daniel; Molnar, Larry; Kinemuchi, Karen; Steenwyk, Steven; Alexander, Cara; Spedden, Chris; Kobulnicky, Henry

    2016-05-01

    Luminous Red Novae (LRN) are rare transient events believed to be caused by the merger of a main sequence contact binary. Since the discovery of the prototype, V838 Mon, only a handful of LRN events have been observed. Tylenda et al. (2011) analyzed the OGLE data preceding the 2008 Novae of V1309 Sco and found that it exhibited a similar light curve to that of a contact binary with one interesting exception, the orbital period of V1309 Sco showed exponential period change going to zero. Unfortunately the system was discovered to be a binary after the merger, preventing any targeted observations to narrow down how the system entered this unusual state. However the extreme period change observed in V1309 Sco gives us a signature to look for in other contact binaries, allowing the discovery of merger candidates for follow up. We will present an analysis of light curves and spectra of KIC 9832227 (NSVS 5597755) that show it is a contact binary system with a negative period derivative that is becoming more extreme with time. These data span more than 15 years and are taken from the NSVS, ASAS, WASP, and Kepler surveys, with ongoing measurements from the Calvin College Observatory and the Apache Point Observatory. The ongoing period change observed in the system is consistent with the exponential model fit from V1309 Sco and the rate of period change has surpassed that of all other measured contact binaries with the exception of V1309 Sco. If the exponential period decay continues the system will likely merge between 2019 and 2022 resulting in a naked eye nova. If this event occurs, this star will present the unprecedented opportunity to study a LRN progenitor and to follow the evolution of the merger.

  14. A transitoriedade: uma nova leitura

    Directory of Open Access Journals (Sweden)

    José Otávio de Vasconcellos Naves

    2008-12-01

    Full Text Available Neste trabalho, o texto de Freud Vergänglichkeit (1916 ganha uma nova perspectiva: é a consciência, transitória, que se ocupa do importante intercâmbio entre o eu e o mundo. Entretanto, ela e a sua transitoriedade adoecem. Na paranóia, ela se perde num futuro aterrador para se reencontrar numa realidade delirante. Na melancolia, a consciência se perde no passado, exaurindo-se na reconstituição de um objeto de desejo impossível de ser considerado como perdido.

  15. Características de carcaça de cordeiros Hampshire Down e Santa Inês sob diferentes fotoperíodos Carcass characteristics of Hampshire Down and Santa Inês ram lambs under different photoperiods

    Directory of Open Access Journals (Sweden)

    José Luiz de Sá

    2005-03-01

    Full Text Available O objetivo deste trabalho foi avaliar o efeito do fotoperíodo e da raça nas características de carcaça de cordeiros machos Hampshire Down e Santa Inês. Sete cordeiros Hampshire Down e sete Santa Inês foram submetidos a fotoperíodo de 12 horas luz x 12 horas escuro (curto e de 18 horas luz x 6 horas escuro (longo. Após o desmame, os cordeiros foram alojados em baias individuais de acordo com os tratamentos. Ao atingirem 31 kg de peso vivo, foram abatidos e a carcaça e os componentes não-constituintes da carcaça foram pesados. Cordeiros Santa Inês apresentaram peso de carcaça quente superior ao dos Hampshire e maior rendimento comercial. Cordeiros Santa Inês apresentaram maior peso de sangue, coração, pulmão, rins e baço. Já os cordeiros Hampshire Down apresentaram pesos de pele, patas e aparelho gastrintestinal cheio superiores aos do Santa Inês. Os cordeiros Santa Inês apresentaram maior largura de garupa e comprimento de perna do que os Hampshire Down. Os cordeiros Santa Inês apresentaram porcentagem de costela descoberta e baixos maior do que os Hampshire Down, com maior porcentagem de perna. A raça influencia mais as características de carcaça do que o fotoperíodo.The objective of this work was to evaluate the effect of photoperiod and breed on carcass characteristics. Seven Hampshire Down and seven Santa Inês ram lambs were assigned to two photoperiods: 12 hours light x 12 hours dark, or short photoperiod, and to 18 hours of light x 6 hours of dark, or long photoperiod. After weaning, the lambs were housed in individual stalls. The lambs were weighed weekly until slaughter weight of 31 kg. After slaughter, the carcass and the non-carcass components were weighed. Santa Inês lambs had higher hot carcass weight than Hampshire Down and also a higher commercial dressing percentage. Santa Inês lambs had higher blood, heart, lung, kidneys and spleen weight. The Hampshire Down lambs had higher skin, feet, full stomach

  16. Avaliação da passagem transplacentária e colostral de cobre e seus principais antagonistas em cordeiros e ovelhas da raça Bergamácia

    OpenAIRE

    Toma, Hugo Shisei [UNESP

    2011-01-01

    Objetivou-se avaliar a passagem transplacentária e colostral de cobre e seus principais antagonistas (Zn, S, Fe e Mo) por meio de dosagem sérica e no colostro, em cordeiros e ovelhas da raça Bergamácia. Foram utilizados 20 cordeiros provenientes de parto simples e suas respectivas mães da raça Bergamácia mantidas confinadas a partir de 15 dias antes do parto, alimentadas com silagem de sorgo, ração, feno, sal mineral e água ad libitum. Foram realizadas colheitas de sangue das mães, por venopu...

  17. Epidemiologia da doença de Chagas no Ceará VIII - estudo da infecção de animais por T. cruzi no município de Morada Nova

    Directory of Open Access Journals (Sweden)

    J. E. Alencar

    1977-02-01

    Full Text Available Foram examinados 1.368 mamíferos em ecótopos naturais ou artificiais: 443 cães com 2,5% positivos; 605 gatos com 0,7%, 65 roedores domésticos com 4,6%, 6 coelhos e 10 cobaias negativos. Dentre os animais silvestres, foram examinados 115 preás (Galea s. spixii com 2,3% positivos, 12 "cassacos" (Didelphis azarae dos quais 9 positivos; 5 quirópteros, 5 punáres (Cercomys c. laurentius e 3 pebas (Dasypus sexcinctus negativos. A amostra apresentada é suficiente para considerada a existência de ciclos doméstico e silvestre de T. cruzi na área estudada e considerada endêmica da Doença de Chagas.

  18. On the Progenitors of Galactic Novae

    CERN Document Server

    Darnley, M J; Bode, M F; Hounsell, R A; Williams, R P

    2011-01-01

    Of the approximately 400 known Galactic classical novae, only ten of them, the recurrent novae, have been seen to erupt more than once. At least eight of these recurrents are known to harbor evolved secondary stars, rather than the main sequence secondaries typical in classical novae. In this paper, we propose a new nova classification system, based solely on the evolutionary state of the secondary, and not (like the current schemes) based on the properties of the outbursts. Using archival optical and near-infrared photometric observations of a sample of thirty eight quiescent Galactic novae we show that the evolutionary state of the secondary star in a quiescent system can predicted and several objects are identified for follow-up observations; CI Aql, V2487 Oph, DI Lac and EU Sct.

  19. Desempenho de cordeiros alimentados com diferentes níveis protéicos Performance of lambs fed with different protein levels

    Directory of Open Access Journals (Sweden)

    Marilice Zundt

    2002-06-01

    Full Text Available O experimento foi conduzido com o objetivo de avaliar níveis crescentes de proteína bruta (PB na dieta de cordeiros em confinamento, por meio de seus efeitos sobre o desempenho animal. Trinta e dois cordeiros "tricross" (¹/2 Texel + ¼ Bergamácia + ¼ Corriedale, sendo 16 machos inteiros e 16 fêmeas, com idade média de 5 meses e peso vivo de 30 kg , foram alimentados durante 57 dias com dietas isoenergéticas (72% NDT, variando os níveis protéicos (12, 16, 20 e 24 % PB. Os animais foram identificados, pesados e distribuídos nos quatro tratamentos. Os cordeiros permaneceram em baias individuais, cobertas, com piso ripado e suspenso. Os parâmetros estudados foram ganho de peso, consumo de matéria seca, conversão alimentar e o custo de produção do quilograma de carcaça. A utilização de dietas, com diferentes níveis protéicos na terminação de cordeiros, mostrou efeito linear positivo para ganho de peso e negativo para conversão alimentar. Verificou-se que a utilização de dietas com níveis protéicos crescentes não influenciou o consumo de matéria seca dos cordeiros. Observou-se viabilidade econômica na terminação de cordeiros, utilizando-se dietas entre 12 e 24% de PB, entretanto, o maior retorno foi obtido com a ração contendo 12% PB. Não houve efeito de sexo para os parâmetros analisados.The experiment was carried out to evaluate increasing crude protein (CP levels in drylot lambs diet, and its effects on animal performance. Thirty two tricross lambs (1/2 Texel + ¼ Bergamácia + ¼ Corriedale, being 16 males and 16 females, with average age 5 months and live weight 30 kg, were fed for 57 days, with isoenergetic diets (72% TDN, but with different protein levels (12, 16, 20 and 24% PB. The animals were identified, weighted and distributed in the four treatments. The lambs were kept underroof in individual pens with lathing and a suspended floor. The studied parameters were weight daily gain, dry matter intake, feed

  20. Qualidade de carnes provenientes de cortes da carcaça de cordeiros e de ovinos adultos Quality of meats from cuts of lamb and adult sheep carcasses

    Directory of Open Access Journals (Sweden)

    Rafael Silvio Bonilha Pinheiro

    2009-09-01

    Full Text Available Com o objetivo de estudar as características qualitativas da carne de ovinos de diferentes categorias quanto aos músculos dos cortes da carcaça (paleta, lombo e perna, utilizaram-se 18 ovinos ½ Ile de France ½ Ideal (seis cordeiros não-castrados, seis ovelhas de descarte e seis machos adultos castrados. Os animais foram criados em pasto de capim-tifton 85 e receberam suplementação (concentrado. Os cordeiros foram abatidos aos 32 kg, com aproximadamente 5 meses de idade, e as ovelhas e os machos adultos castrados, com 55 kg e aos 60 meses de idade. Não houve diferenças nos valores de pH 45 minutos e pH 24 horas entre as categorias animais e nos músculos dos cortes da carcaça. A idade de abate influenciou a luminosidade da carne de todos os músculos. O teor de vermelho não diferiu entre os animais adultos, mas foi superior aos valores obtidos na carne dos cordeiros. A carne de animais adultos é mais escura que a de cordeiros. As perdas por cocção no músculo Triceps brachii são maiores que no Longissimus lumborum e Semimembranosus. Os valores de pH e a capacidade de retenção de água são similares entre as categorias animais.Eighteen ½ Ile de France ½ Polwarth sheep (6 no castrated lambs, 6 discarded ewes and 6 discarded wethers were used to evaluate qualitative traits of meat from different categories of sheep for muscle cuts (shoulder, loin and leg. The animals were raised in grazing system with tifton-85 pastures and supplemented with concentrate. Lambs were slaughtered at 32 kg body weight, close to 5 months of age. Ewes and wethers were slaughtered with 55 kg and 60 months of age. There were no differences in pH45mim and pH24h values among different animal categories and muscles of carcass cuts. There was difference in meat luminosity between lambs and adult animals, considering all the evaluated muscles. The red level did not differ between adult categories, but it was higher than values observed in lambs. In

  1. Glicerina bruta no suplemento para cordeiros lactentes em pastejo de azevém Crude glycerin in supplement to suckling lambs on ryegrass pasture

    Directory of Open Access Journals (Sweden)

    Ana Carolina Ribeiro Sanquetta de Pellegrin

    2012-08-01

    Full Text Available Avaliou-se o efeito de níveis de glicerina bruta sobre o consumo de suplemento e o desempenho de cordeiros lactentes mantidos a pasto, além das características quali-quantitativas do pasto de azevém. Foram utilizados 32 cordeiros lactentes distribuídos nos tratamentos: 0, 10, 20 e 30% de glicerina bruta, em substituição ao milho, no suplemento isoproteico (18% PB fornecido diariamente em quantidade equivalente a 2% do peso corporal. Não houve efeito (P>0,05 dos níveis de glicerina bruta sobre as características qualitativas e quantitativas do pasto, na composição de proteína bruta e fibra detergente neutro e na carga animal suportada pela pastagem, nem no consumo de suplemento, ganho de peso médio diário e o número de dias até o abate dos cordeiros. Níveis de até 30% de glicerina bruta, em substituição ao milho, no suplemento fornecido para cordeiros lactentes pastejando azevém não comprometem o consumo de suplemento, desempenho e período de terminação dos animais.The aim of this study was to evaluate the effect of levels of crude glycerin in the supplement intake and performance of suckling lambs on ryegrass pasture, beyond the qualitative and quantitative characteristics of ryegrass pastures. It was used 32 suckling lambs distributed between the treatments: 0, 10, 20 and 30% of crude glycerin, replacing corn, in the isoproteic supplement (18% CP offered daily in an amount equivalent to 2% of body weight. There was no effect (P>0.05 of the levels of crude glycerin on the qualitative and quantitative characteristics of pastures, composition of crude protein and neutral detergent fiber, stocking rate supported by ryegrass pasture, neither on supplement intake, average weight gain and number of days to slaughter the lambs. Levels up to 30% of crude glycerin, replacing corn, provided in the supplement to suckling lambs grazing ryegrass didn't compromise the supplement intake, performance and termination period of the

  2. The NOvA Technical Design Report

    Energy Technology Data Exchange (ETDEWEB)

    Ayres, D.S.; Drake, G.R.; Goodman, M.C.; Grudzinski, J.J.; Guarino, V.J.; Talaga, R.L.; Zhao, A.; /Argonne; Stamoulis, P.; Stiliaris, E.; Tzanakos, G.; Zois, M.; /Athens U. /Caltech /UCLA /Fermilab /College de France /Harvard U. /Indiana U. /Lebedev Inst. /Michigan State U. /Minnesota U., Duluth /Minnesota U.

    2007-10-08

    Technical Design Report (TDR) describes the preliminary design of the NOvA accelerator upgrades, NOvA detectors, detector halls and detector sites. Compared to the March 2006 and November 2006 NOvA Conceptual Design Reports (CDR), critical value engineering studies have been completed and the alternatives still active in the CDR have been narrowed to achieve a preliminary technical design ready for a Critical Decision 2 review. Many aspects of NOvA described this TDR are complete to a level far beyond a preliminary design. In particular, the access road to the NOvA Far Detector site in Minnesota has an advanced technical design at a level appropriate for a Critical Decision 3a review. Several components of the accelerator upgrade and new neutrino detectors also have advanced technical designs appropriate for a Critical Decision 3a review. Chapter 1 is an Executive Summary with a short description of the NOvA project. Chapter 2 describes how the Fermilab NuMI beam will provide a narrow band beam of neutrinos for NOvA. Chapter 3 gives an updated overview of the scientific basis for the NOvA experiment, focusing on the primary goal to extend the search for {nu}{sub {mu}} {yields} {nu}{sub e} oscillations and measure the sin{sup 2}(2{theta}{sub 13}) parameter. This parameter has not been measured in any previous experiment and NOvA would extend the search by about an order of magnitude beyond the current limit. A secondary goal is to measure the dominant mode oscillation parameters, sin{sup 2}(2{theta}{sub 23}) and {Delta}m{sub 32}{sup 2} to a more precise level than previous experiments. Additional physics goals for NOvA are also discussed. Chapter 4 describes the Scientific Design Criteria which the Fermilab accelerator complex, NOvA detectors and NOvA detector sites must satisfy to meet the physics goals discussed in Chapter 3. Chapter 5 is an overview of the NOvA project. The changes in the design relative to the NOvA CDR are discussed. Chapter 6 summarizes the NOvA

  3. Searching for nova shells around cataclysmic variables

    CERN Document Server

    Sahman, D I; Knigge, C; Marsh, T R

    2015-01-01

    We present the results of a search for nova shells around 101 cataclysmic variables (CVs), using Halpha images taken with the 4.2-m William Herschel Telescope (WHT) and the 2.5-m Isaac Newton Telescope Photometric Halpha Survey of the Northern Galactic Plane (IPHAS). Both telescopes are located on La Palma. We concentrated our WHT search on nova-like variables, whilst our IPHAS search covered all CVs in the IPHAS footprint. We found one shell out of the 24 nova-like variables we examined. The newly discovered shell is around V1315 Aql and has a radius of approx.2.5 arcmin, indicative of a nova eruption approximately 120 years ago. This result is consistent with the idea that the high mass-transfer rate exhibited by nova-like variables is due to enhanced irradiation of the secondary by the hot white dwarf following a recent nova eruption. The implications of our observations for the lifetime of the nova-like variable phase are discussed. We also examined 4 asynchronous polars, but found no new shells around an...

  4. Medium-band photometry of novae

    Energy Technology Data Exchange (ETDEWEB)

    Yao, B.A.; Mo, J.E.

    1975-06-01

    In the early stage of novae, the conventional method of photometric transformation is accepted. When the novae are in a nebular stage, one cannot assign the observed values as U, B, V, whether one reduces them by photometric transformation or not. A quantitative calculation was made by means of spectral datum. It proves that the result of the observation may lead to unexpected differences. Differential extinction also cannot be corrected by the conventional method. Some suggestions for better observation and reduction of novae photometry are given.

  5. Effects of crossbreeding on carcass and meat quality of Mexican lambs Efeito do cruzamento sobre o rendimento de carcaça e a qualidade da carne de cordeiros mexicanos

    Directory of Open Access Journals (Sweden)

    L. Hernández-Cruz

    2009-04-01

    Full Text Available Twenty hair (Pelibuey x Katadin x BlackBelly and 20 wool (Rambouillet x Criollo lambs were fattened in an intensive feeding system to reach 40kg body weight at ten months of age. The yield of lamb sides and back fat (51.9%, 2.5mm vs. 47.0%, 2.3mm were greater in wool lambs. Meat pH was not different between phenotypes but meat temperature was higher during the first hours postmortem in wool lamb sides (27, 23, and 20, vs. 24, 20, and 17ºC. Protein content in meat from the neck (braquicephalic and esternocephalic muscles and loin (Longissimus lumborum muscle were higher in hair lambs (21.1 and 20.4 vs. 19.7 and 19.3 %, while moisture of the same muscles was higher in wool lambs (75.6 and 75.9 vs. 73.6 and 74.3%. Ash content was similar in both phenotypes, but palmitoleic acid was greater in hair lambs (2.9 and 2.7 vs. 2.7 and 2.5%. In fresh meat, pH, meat toughness, and water activity (Wa of loin did not differ; but water holding capacity (WHC was higher in hair lambs, and the same response was observed for cooked meat toughness from the neck, and in raw and cooked meat from loin. There were differences in the colour of meat from the neck, having values for L*, b* and tonalities greater in wool lambs, and a* greater for hair lambs. Sensorial parameters were similar in both phenotypes.Vinte cordeiros deslanados (Pelibuey x Katadin x BlackBelly e 20 cordeiros lanados (Rambouillet x Criollo foram mantidos em um sistema intensivo de alimentação até atingirem 40kg, aos 10 meses de idade. O rendimento de carcaça e a espessura da gordura foram maiores nos cordeiros lanados (51,9%, 2,5mm vs. 47,0%, 2,3mm. Não houve diferenças entre os dois grupos de cordeiros para pH, mas a temperatura da carne foi mais alta durante as primeiras horas pós-morte, nas meias-carcaças dos cordeiros lanados (27, 23, 20 vs. 24, 20, 17°C. O conteúdo proteico da carne do pescoço (músculos braquicefálico e esternocefálico e do lombo (músculo Longissimus lumborum

  6. On Orbital Period Changes in Nova Outbursts

    CERN Document Server

    Martin, Rebecca G; Schaefer, Bradley E

    2011-01-01

    We propose a new mechanism that produces an orbital period change during a nova outburst. When the ejected material carries away the specific angular momentum of the white dwarf, the orbital period increases. A magnetic field on the surface of the secondary star forces a fraction of the ejected material to corotate with the star, and hence the binary system. The ejected material thus takes angular momentum from the binary orbit and the orbital period decreases. We show that for sufficiently strong magnetic fields on the surface of the secondary star, the total change to the orbital period could even be negative during a nova outburst, contrary to previous expectations. Accurate determinations of pre- and post-outburst orbital periods of recurrent nova systems could test the new mechanism, in addition to providing meaningful constraints on otherwise difficult to measure physical quantities. We apply our mechanism to outbursts of the recurrent nova U Sco.

  7. The Terra Nova oil field development

    Energy Technology Data Exchange (ETDEWEB)

    Bruce, G.C. [Petro-Canada, Inc., St. John' s, NF (Canada)

    2001-07-01

    Before expanding on the development of the Terra Nova oilfield, the author discussed the overall business strategy of Petro-Canada and identified where the Terra Nova and offshore Newfoundland oil have their place within this strategy. The principal basins and oilfields offshore Newfoundland were reviewed, then the emphasis shifted to rest on the Terra Nova development project. A whole range of topics were brought up, including the Floating Production, Storage and Offloading (FPSO) facility, the modules layout, the FPSO located at Bull Arm, and the floating production systems. The physical environment of the Grand Banks was highlighted, and the next few sections were devoted to the Terra Nova FPSO, FPSO and drill centres, the Turret General Arrangement, and Spider buoy including the disconnect/reconnect. The last four sections dealt with the animation of riser movement, the wellhead protection animation, Henry Goodrich, and operations readiness.

  8. Desenvolvimento relativo dos tecidos ósseo, muscular e adiposo dos cortes da carcaça de cordeiros Santa Inês

    Directory of Open Access Journals (Sweden)

    Santos Cristiane Leal dos

    2001-01-01

    Full Text Available O trabalho foi conduzido no Setor de Ovinocultura do Departamento de Zootecnia da UFLA, em Lavras, com o objetivo de estudar o crescimento alométrico dos tecidos ósseo, muscular e adiposo dos cortes comerciais em cordeiros. Foram utilizados 24 cordeiros machos inteiros da raça Santa Inês. Os animais foram submetidos a regime de confinamento e receberam alimentação ad libitum. O abate ocorreu quando os animais atingiram os pesos vivos de 15, 25, 35 e 45 kg. Após a carcaça ter sido limpa e resfriada, foram obtidos os cortes comerciais a partir da meia carcaça esquerda. A quantidade dos diferentes tecidos foram obtidos por intermédio da dissecação de perna, lombo, costeleta, costela/ fralda e paleta. O estudo do desenvolvimento relativo da composição tecidual foi feito por meio do modelo de HUXLEY (1932. Constatou-se crescimento heterogônico negativo (b 1 para o tecido adiposo de todos os cortes. Quanto ao tipo de crescimento do tecido muscular da costela/fralda e paleta, foi verificado crescimento isogônico (b=1 deste tecido em relação aos cortes.

  9. Chacal ou Cordeiro? O Brasil frente aos desafios e oportunidades do Sistema Internacional Jackal or Lamb? Brazil in face of the challenges and opportunities of the International System

    Directory of Open Access Journals (Sweden)

    Júlio César Cossio Rodriguez

    2012-12-01

    Full Text Available Este artigo analisa as configurações da política externa brasileira pós-2002 para relacionar os ganhos e perdas com as mudanças estruturais do sistema internacional. O intuito e realizar um balanço das capacidades materiais do Brasil, assim como dos seus desafios e oportunidades, a partir das categorias propostas por Randall Schweller. Chacal ou Cordeiro? Como se comporta o Brasil num sistema internacional em transição e quais podem ser as consequências? Ou seja, atua como chacal na busca de ganhos relativos ao seguir o ator mais revisionista (China, e como cordeiro na associação direta com a potência unipolar.This article analyzes the configurations of Brazilian foreign policy after 2002 in order to relate to gains and losses the structural changes of the international system. The aim is to achieve a balance of material capabilities of Brazil, as well as its challenges and opportunities, from the categories proposed by Randall Schweller. Jackal or Lamb? How does Brazil behave in the international system in transition, and what can be the consequences? That is, while Jackal it acts in pursuit of relative gains by following the more revisionist actor (China, and as Lamb in direct association with the unipolar power.

  10. The Effect of Composition on Nova Ignitions

    CERN Document Server

    Shen, Ken J

    2008-01-01

    The accretion of hydrogen-rich matter onto C/O and O/Ne white dwarfs in binary systems leads to unstable thermonuclear ignition of the accreted envelope, triggering a convective thermonuclear runaway and a subsequent classical, recurrent, or symbiotic nova. Prompted by uncertainties in the composition at the base of the accreted envelope at the onset of convection, as well as the range of abundances detected in nova ejecta, we examine the effects of varying the composition of the accreted material. For high accretion rates and carbon mass fractions 0.002. These different triggering mechanisms, which occur for critical abundances relevant to many nova systems, alter the amount of mass that is accreted prior to a nova, causing the nova rate to depend on accreted composition. Upcoming deep optical surveys such as Pan-STARRS-1, Pan-STARRS-4, and the Large Synoptic Survey Telescope may allow us to detect the dependence of nova rates on accreted composition. Furthermore, the burning and depletion of 3He with a mas...

  11. Fontes de óleo vegetal na dieta de cordeiros em confinamento Vegetable oil sources in feedlot lambs

    Directory of Open Access Journals (Sweden)

    Sandra Mari Yamamoto

    2005-04-01

    Full Text Available Objetivou-se avaliar a ingestão de matéria seca, o ganho de peso diário, a conversão alimentar, o peso vivo ao abate e o período de confinamento em cordeiros Santa Inês puros e ½Dorset ½Santa Inês, alimentados com dietas isoenergéticas (76,59% de NDT e isoprotéicas (17,48% de PB contendo diferentes fontes de óleo vegetal (óleos de soja, canola e linhaça e uma dieta controle (sem inclusão de óleo vegetal. A relação volumoso:concentrado foi de 30:70 e utilizou-se feno de aveia como volumoso. Realizou-se também um ensaio de digestibilidade, utilizando quatro cordeiros não-castrados, distribuídos em delineamento quadrado latino, avaliando-se ingestão, excreção fecal e digestibilidade total dos nutrientes das rações. A ingestão de matéria seca, expressa em porcentagem do peso vivo, foi menor nos cordeiros que receberam dieta contendo óleo de canola que naqueles que receberam dieta controle. Porém, todas as rações proporcionaram ganhos de peso e conversão alimentar satisfatórios. Os valores de digestibilidade total da matéria seca (76,02% e matéria orgânica (76,82% da dieta controle foram superiores aos da dieta contendo óleo de linhaça (72,11% e 72,97%, respectivamente, embora não tenham diferido das dietas contendo óleos de soja (72,94 e 73,71% e canola (73,45 e 74,25%. A digestibilidade do extrato etéreo foi menor na dieta controle (84,02%, enquanto as demais dietas apresentaram valor médio de 91,98%. Os óleos vegetais reduziram a digestibilidade da matéria seca e da matéria orgânica, não afetando a ingestão e digestão dos demais nutrientes.This experiment was carried out to evaluate the dry matter ingestion, average daily gain, feed:gain ratio, live weight at slaughter and days in trial in pure Santa Inês and ½Dorset ½Santa Inês lambs, submitted to isoenergetic (76.59% TDN and isoprotein (17.48% crude protein diets with different sources of vegetable oil (soybean oil, canola and linseed and a

  12. Atmospheric deposition 2000. NOVA 2003; Atmosfaerisk deposition 2000. NOVA 2003

    Energy Technology Data Exchange (ETDEWEB)

    Ellermann, T.; Hertel, O.; Hovmand, M.F.; Kemp, K.; Skjoeth, C.A.

    2001-11-01

    This report presents measurements and calculations from the atmospheric part of NOVA 2003 and covers results for 2000. It summarises the main results concerning concentrations and depositions of nitrogen, phosphorus and sulphur compounds related to eutrophication and acidification. Depositions of atmospheric compounds to Danish marine waters as well as land surface are presented. Measurements: In 2000 the monitoring program consisted of eight stations where wet deposition of ammonium, nitrate, phosphate (semi quantitatively) and sulphate were measured using bulk precipitation samplers. Six of the stations had in addition measurements of atmospheric content of A, nitrogen, phosphorus, and sulphur compounds in gas and particulate phase carried out by use of filter pack samplers. Filters were analysed at the National Environmental Research Institute. Furthermore nitrogen dioxide were measured using nitrogen dioxide filter samplers and monitors. Model calculations: The measurements in the monitoring program were supplemented with model calculations of concentrations and depositions of nitrogen and sulphur compounds to Danish land surface, marine waters, fjords and bays using the ACDEP model (Atmospheric Chemistry and Deposition). The model is a so-called trajectory model and simulates the physical and chemical processes in the atmosphere using meteorological and emission data as input. The advantage of combining measurements with model calculations is that the strengths of both methods is obtained. Conclusions concerning: 1) actual concentration levels at the monitoring stations, 2) deposition at the monitoring stations, 3) seasonal variations and 4) long term trends in concentrations and depositions are mainly based on the direct measurements. These are furthermore used to validate the results of the model calculations. Calculations and conclusions concerning: 1) depositions to land surface and to the individual marine water, 2) contributions from different emission

  13. Novas tecnologias, novas competências New Tecnologies, new skills

    Directory of Open Access Journals (Sweden)

    Geneviève Jacquinot Delaunay

    2008-01-01

    Full Text Available O texto aborda a relação dos jovens e adolescentes com tecnologias, nem "novas" nem "velhas", e sim instrumentos para informar e comunicar, divertir, auxiliar nos trabalhos escolares. Apesar de reconhecer a familiaridade dessa geração com o que há de mais avançado em termos de tecnologia, aponta a necessidade de se compreender a complexidade desse novo cenário de aprendizagem, que envolve o aprofundamento de conceitos como interatividade e interação, linguagem numérica, multimídia, internet e hipertexto. Na seqüência, faz uma análise do contato dos jovens com essa diversidade de meios, suas implicações no processo cognitivo e suas conseqüências comunicacionais. Finalmente, reconhece que a aprendizagem é hipercomplexa e que - apesar de todo avanço científico - a máquina, mesmo interativa, não pode proporcionar ao indivíduo o aprendizado que lhe proporciona a interação com outras pessoas.The paper discusses how young people relate to technology, not seen as new or old, but as an instrument to communicate and keep informed, amuse and to help in school projects. Although it is clear that the new generations are much more familiarized with new technology, the focus is on the need to understand the complexity of the new scenario, which requires a deeper understanding of the concepts of interactivity, multimedia, internet and hypertext. It is discussed how young people enter in contact with this diversity of instruments. It is stressed, however, that no matter how complex the computer can be, nothing can replace the role of interacting with other people in the learning process.

  14. Uma nova forma de Coffea

    Directory of Open Access Journals (Sweden)

    C. A. Krug

    1950-01-01

    Full Text Available Nos extensos trabalhos de melhoramento do cafeeiro, há 18 anos em realização na Subdivisão de Genética do Instituto Agronômico, tem-se dedicado especial atenção à espécie C. arabica L., pelo fato de todos os nossos cafèzais pertencerem a esta espécie que, sem dúvida, fornece o produto de melhor qualidade. Nas regiões de terras extremamente cansadas, um dos principais fatôres levados em consideração no melhoramento é a rusticidade, caráter êsse, entretanto, encontrado de preferência em outras espécies, tais como o C. canephora e C. Dewevrei, cujos cafés são de má qualidade. A hibridação interespecífica, que poderia reunir em uma só planta caraterísticos de rusticidade e boa qualidade de bebida, tem o inconveniente de dar origem a plantas triplóides, que são estéreis. Daí se deduz que a obtenção artificial de formas que combinassem êsses caraterísticos constitui problema, cuja solução é extremamente demorada. No presente trabalho, apresentam-se os caracteres de uma nova forma de Coffea, encontrada em cafèzal da Fazenda Itaporã, em Terra Roxa, município de Viradouro, que, com algumas ressalvas, oferece a desejada combinação de caracteres. Trata-se, provàvelmente, de um híbrido espontâneo entre C. arabica e C. Dewevrei, com 2n = 44 cromosômios, extremamente rústico e produtivo, cujas sementes fornecem uma bebida que pode ser classificada como boa. Apenas apresenta, como principal defeito, uma auto-esterilidade quase completa. Os seus caraterísticos botânicos são descritos em detalhe. Devido ao seu porte elevado, ramos abundantes e folhas grandes e coriáceas, esse cafeeiro se assemelha ao C. Dewevrei. Os frutos são oval-elípticos, de um vermelho bem escuro quando maduros, e as sementes oblongas, constatan-do-se elevada percentagem do tipo "moca" e "chocha". Quanto à constituição citológica, as pesquisas conduziram à hipótese de este cafeeiro possuir 22 cromosômios de C. arabica e 22 (n

  15. When does an old nova become a dwarf nova? Kinematics and age of the nova shell of the dwarf nova AT Cancri

    Science.gov (United States)

    Shara, Michael M.; Drissen, Laurent; Martin, Thomas; Alarie, Alexandre; Stephenson, F. Richard

    2017-02-01

    The Z Cam-type dwarf nova AT Cancri (AT Cnc) displays a classical nova (CN) shell, demonstrating that mass transfer in cataclysmic binaries decreases substantially after a CN eruption. The hibernation scenario of cataclysmic binaries predicts such a decrease, on a time-scale of a few centuries. In order to measure the time since AT Cnc's last CN eruption, we have measured the radial velocities of a hundred clumps in its ejecta with SITELLE, Canada-France-Hawaii Telescope's recently commissioned imaging Fourier transform spectrometer. These range from -455 to +490 km s-1. Coupled with the known distance to AT Cnc of 460 pc, the size of AT Cnc's shell, and a simple model of nova ejecta deceleration, we determine that the last CN eruption of this system occurred 330_{-90}^{+135} yr ago. This is the most rapid transition from a high mass-transfer rate, nova-like variable to a low mass-transfer rate, dwarf nova yet measured, and in accord with the hibernation scenario of cataclysmic binaries. We conclude by noting the similarity in the deduced outburst date (within a century of 1686 CE) of AT Cnc to a `guest star' reported in the constellation Cancer by Korean observers in 1645 CE.

  16. Gamma-ray emission from nova outbursts

    CERN Document Server

    Hernanz, M

    2013-01-01

    Classical novae produce radioactive nuclei which are emitters of gamma-rays in the MeV range. Some examples are the lines at 478 and 1275 keV (from 7Be and 22Na) and the positron-electron annihilation emission, with the 511 keV line and a continuum. Gamma-ray spectra and light curves are potential unique tools to trace the corresponding isotopes and to give insights on the properties of the expanding envelope. Another possible origin of gamma-rays is the acceleration of particles up to very high energies, so that either neutral pions or inverse Compton processes produce gamma-rays of energies larger than 100 MeV. MeV photons during nova explosions have not been detected yet, although several attempts have been made in the last decades; on the other hand, GeV photons from novae have been detected with the Fermi satellite in V407 Cyg, a nova in a symbiotic binary, where the companion is a red giant with a wind, instead of a main sequence star as in the cataclysmic variables hosting classical novae. Two more nov...

  17. Gamma-ray Novae: Rare or Nearby?

    CERN Document Server

    Morris, Paul J; Brown, Anthony M; Chadwick, Paula M

    2016-01-01

    Classical Novae were revealed as a surprise source of gamma-rays in Fermi LAT observations. During the first 8 years since the LAT was launched, 6 novae in total have been detected to > 5 sigma in gamma-rays, in contrast to the 69 discovered optically in the same period. We attempt to resolve this discrepancy by assuming all novae are gamma-ray emitters, and assigning peak one-day fluxes based on a flat distribution of the known emitters to a simulated population. To determine optical parameters, the spatial distribution and magnitudes of bulge and disc novae in M31 are scaled to the Milky Way, which we approximate as a disc with a 20 kpc radius and elliptical bulge with semi major axis 3 kpc and axis ratios 2:1 in the xy plane. We approximate Galactic reddening using a double exponential disc with vertical and radial scale heights of r_d = 5 kpc and z_d = 0.2 kpc, and demonstrate that even such a rudimentary model can easily reproduce the observed fraction of gamma-ray novae, implying that these apparently r...

  18. Características das carcaças e componentes do peso vivo de cordeiros terminados em pastagem ou confinamento = Carcass characteristics and live weight components in lambs finished on pasture or feedlot

    Directory of Open Access Journals (Sweden)

    Maria Angela Machado Fernandes

    2008-01-01

    Full Text Available O trabalho objetivou avaliar as características da carcaça e os não-componentes da carcaça de cordeiros em quatro sistemas: cordeiros desmamados aos 60 dias mantidos em pastagem; cordeiros + ovelhas em pastagem; cordeiros + ovelhas em pastagem + concentrado em creep feeding (1% PV; cordeiros desmamados aos 60 dias e confinados. Os cordeiros foram abatidos quando a média de peso vivo do tratamento alcançou entre 32-34 kg. Após o abate, foram coletados e pesados os não-componentes da carcaça. Obtiveram-se pesos, rendimentos emedidas objetivas das carcaças e por cálculos a compacidade de perna e carcaça. A metodologia para determinar o momento de abate promoveu grande variação (7 a 14 kg no peso vivo final entre os animais do mesmo tratamento. Houve correlação significativa (p This experiment had the objective to evaluate the carcass characteristics and the non-carcass components of lambs on four systems: lambs weaned at 60 days of age kept on pasture; lambs + ewes kept on pasture; lambs + ewe + concentrate in creep feeding; lambs weaned at 60 days and kept on feedlot. Lambs were slaughteredwhen mean live weight from the tratament reached 32-34 kg. After slaughter, the noncarcass components were collected and weighed. The weight, yield and carcass measures were obtained, while leg and carcass compacity was calculated. The elected methodology fordetermining slaughter time resulted in large variation (7 to 14 kg in the slaughter weight of lambs from the same treatments. There was a significant (p < 0.05 positive correlation between hot (r = 0.83 and cold (r = 0.85 carcass weights, and slaughtered weight. Lambsweaned and finished on pasture showed lower (p < 0.05 hot carcass dressing (42.3%, cold carcass dressing (40.2%, carcass biological dressing (51.8% and thorax width (22.99 cm and higher (p < 0.05 gastrointestinal content (5.6 kg. The presence of dams had aninfluence in systems were there was no weaning, in regard to carcass

  19. Consumo, desempenho e análise econômica da alimentação de cordeiros terminados em confinamento com o uso de dietas de alto grão

    Directory of Open Access Journals (Sweden)

    G.M.C. Bernardes

    2015-12-01

    Full Text Available O presente experimento, conduzido no Laboratório de Ovinocultura da Universidade Federal de Santa Maria, teve como objetivo avaliar o efeito do uso de diferentes dietas de alto grão sobre o consumo de nutrientes e o desempenho de cordeiros terminados em confinamento, bem como realizar uma análise econômica da alimentação utilizada para terminação dos animais. Foram utilizados 32 cordeiros machos, castrados, da raça Texel, nascidos de parto simples e desmamados com aproximadamente 50 dias de idade. Os tratamentos foram constituídos por diferentes tipos de grãos, não processados, sendo: grão de milho, grão de aveia branca, grão de aveia preta ou grão de arroz com casca. Os animais foram abatidos quando atingiram o peso vivo de abate pré-estabelecido de 32kg, que corresponde a 60% do peso adulto de suas mães. Cordeiros alimentados com dietas de alto grão de milho apresentam maiores consumos de matéria seca, matéria orgânica, proteína bruta, carboidratos totais e de nutrientes digestíveis totais, menor consumo de fibra em detergente neutro, melhor escore de condição corporal, ganho de peso e conversão alimentar, o que leva à redução do número de dias no confinamento necessários para atingir o peso de abate. Além disso, cordeiros terminados com o uso de dieta de alto grão à base de grão de milho proporcionam melhor resultado econômico quando comparados com cordeiros terminados com as demais dietas de alto grão utilizadas neste experimento. O uso de dietas de alto grão de milho, aveia branca, aveia preta ou arroz com casca para terminação de cordeiros em sistema de confinamento é uma alternativa viável do ponto de vista produtivo. Porém, o uso de grão de milho proporciona melhores resultados produtivos e econômicos.

  20. Produção de cordeiros da raça Suffolk em dois sistemas de manejo reprodutivos Suffolk lambs production in two mating systems

    Directory of Open Access Journals (Sweden)

    Domingos Sanchez Roda

    1999-03-01

    Full Text Available Foram utilizadas 32 ovelhas Suffolk por dois anos, em dois sistemas de monta, com acasalamentos a cada oito meses (alternativo ou a cada doze meses (tradicional, visando a reduzir a estacionalidade da disponibilidade de animais para abate. Não foram observadas diferenças (P>0,05 na fertilidade e prolificidade dos animais, sendo no sistema alternativo, 66,7% e 110,4% e no tradicional 78,1%; 103,1% , obtendo-se 53 e 33 crias nascidas no período, respectivamente. Para a mortalidade das crias, observou-se, respectivamente, 28,3% e 6,1% (P0,05 e o peso da ovelha à parição foi de 68,06 e 71,05kg (P>0,05, para o sistema alternativo e tradicional, respectivamente. Conclui-se que o sistema de monta alternativo possibilita a obtenção de maior número de cordeiros, sem prejuízo no desempenho ponderal das ovelhas e dos cordeiros, bem como uma melhor distribuição na produção de cordeiros para abate durante o ano.Thirty-two Suffolk ewes were utilized for two years in two different mating systems: a traditional (mating at every twelve months and an alternative (at every eight months, aimed to reduce the seasonality of available animal to slaughter. The fertility and prolificity of ewes in the alternative system were 66.7 and 110.4% and in the traditional system 76.1 and 103.1%. It was obtained 53 and 33 lambs in the period. Lamb mortality were 28.3 and 6.1% (P0.05 and parturition ewe weight were 66.06 and 71.05kg (P>0.05 for alternative and traditional system, respectively. Alternative mating system made possible to obtain larger number of lambs, without deleteriou effect to ewes and lambs performances, as well as a better distribution in the number of lamb for slaughter during the year.

  1. The Expanding Fireball of Nova Delphini 2013

    CERN Document Server

    Schaefer, G H; Gies, D R; Farrington, C D; Kloppenborg, B; Chesneau, O; Monnier, J D; Ridgway, S T; Scott, N; Tallon-Bosc, I; McAlister, H A; Boyajian, T; Maestro, V; Mourard, D; Meilland, A; Nardetto, N; Stee, P; Sturmann, J; Vargas, N; Baron, F; Ireland, M; Baines, E K; Che, X; Jones, J; Richardson, N D; Roettenbacher, R M; Sturmann, L; Turner, N H; Tuthill, P; van Belle, G; von Braun, K; Zavala, R T; Banerjee, D P K; Ashok, N M; Joshi, V; Becker, J; Muirhead, P S

    2015-01-01

    A classical nova occurs when material accreting onto the surface of a white dwarf in a close binary system ignites in a thermonuclear runaway. Complex structures observed in the ejecta at late stages could result from interactions with the companion during the common envelope phase. Alternatively, the explosion could be intrinsically bipolar, resulting from a localized ignition on the surface of the white dwarf or as a consequence of rotational distortion. Studying the structure of novae during the earliest phases is challenging because of the high spatial resolution needed to measure their small sizes. Here we report near-infrared interferometric measurements of the angular size of Nova Delphini 2013, starting from one day after the explosion and continuing with extensive time coverage during the first 43 days. Changes in the apparent expansion rate can be explained by an explosion model consisting of an optically thick core surrounded by a diffuse envelope. The optical depth of the ejected material changes ...

  2. NOVA laser facility for inertial confinement fusion

    Energy Technology Data Exchange (ETDEWEB)

    Simmons, W.W.

    1983-11-30

    The NOVA laser consists of ten beams, capable of concentrating 100 to 150 kJ of energy (in 3 ns) and 100 to 150 TW of power (in 100 ps) on experimental targets by 1985. NOVA will also be capable of frequency converting the fundamental laser wavelength (1.05 ..mu..m) to its second (0.525 ..mu..m) or third (0.35 ..mu..m) harmonic. This additional capability (80 to 120 kJ at 0.525 ..mu..m, 40 to 70 kJ at 0.35 ..mu..m) was approved by the US Department of Energy (DOE) in April 1982. These shorter wavelengths are much more favorable for ICF target physics. Current construction status of the NOVA facility, intended for completion in the autumn of 1984, will be presented.

  3. Enquête de satisfaction Novae

    CERN Multimedia

    2014-01-01

    Novae lance une enquête de satisfaction auprès de ses clients. Vous pouvez accéder au questionnaire au sujet des trois restaurants d’entreprise du CERN en utilisant le lien et les codes ci-dessous. Le délai de réponse est fixé au jeudi 29 mai.   https://survey.mis-trend.ch/NOVAE Voici les codes à introduire (en respectant la casse) pour entrer dans le questionnaire, selon le site : CERN Restaurant n°1 : CERN114 CERN Restaurant n°2 : CERN214 CERN Restaurant n°3 : CERN314   Nous attirons votre attention sur le fait que tout questionnaire rempli sera validé. Nous vous prions donc de ne pas utiliser ce lien pour tester le questionnaire. Merci d’avance pour votre collaboration. L'équipe Novae

  4. Um novo paradigma para uma nova antropologia

    Directory of Open Access Journals (Sweden)

    Susin, Luiz Carlos

    2007-01-01

    Full Text Available Este artigo recolhe relativas à identidade humana no contexto das pesquisas científicas e das transformações ocorridas nos últimos tempos, especialmente no século XX. A nova fisica, com um novo desenho do universo, uma nova cosmologia, radicaliza, por um lado, as questões em torno do humano, e, por outro lado, abre novas possibilidades. Um novo paradigma, mais holístico, incluindo a dimensão ecológica, ou ao menos com cenários mais adequados, pode ser vislumbrado, embora ainda não descrito, por estarmos numa "era de transição". Na parte que nos toca no universo - a terra - o futuro da vida depende, em grande parte, de decisões éticas que somente o ser humano é convocado a assumir

  5. Nova variedade de Menta arvensis

    Directory of Open Access Journals (Sweden)

    Abelardo Rodrigues Lima

    1952-09-01

    Full Text Available No quarto ano dos trabalhos de seleção com a menta japonêsa, foi encontrado um "seedling", o M. A. 701, que se destacou pela resistência à ferrugem e pela sua rusticidade. Os caracteres botânicos dessa variedade comercial, principalmente hábito vegetativo, coloração das fôlhas e das hastes, a tornam completa' mente distinta da variedade original. Esta distinção se confirma e acentua quando se compara a natureza dos componentes do óleo essencial da menta "Campinas" M. A. 701, descrita no presente trabalho, com a menta japonêsa comum. A maior produtividade da nova variedade comparada com a da menta japonesa comum foi desde logo também constatada pelos primeiros lavradores, a quem foram enviadas pequenas quantidades de rizomas, para plantio experimental. Foram cultivados em 1949-50 cêrca de 12 hectares; cm 1950-51, cêrca de 900 ha, e o prognóstico é que essa variedade tende a substituir totalmente a menta japonêsa anteriormente cultivada em São Paulo, devido ao seu maior valor econômico.A seedling, designated M.A.701, remarkable for its vigor and resistance to rust, was discovered during the fourth year of selection of Japanese mint (Mentha arvensis L. subsp. haplocalix Briquet var. piperascens Holmes or forma piperascens Malinvaud. The botanical characters of the variety derived from this seedling, especially the vegetative habit and colouring of leaves and stems, make it quite different from the original variety. This difference is enhanced, when we compare the nature of the essential oil components of "Campinas" M.A.701, as described in the present paper, with that of the common Japanese mint. The higher yield of the new variety, compared with that of the common Japanese mint, was soon confirmed by the first cultivators, to whom small quantities of rhizomes were sent for experimental planting. About 12 hectars were cultivated em 1949/50 and about 900 hectars in 1950/51. It is expected that the new variety will, on account

  6. Novas cartas portuguesas: uma abordagem feminista

    OpenAIRE

    Jesus, Isabel Henriques de

    2012-01-01

    Publicado em 1972 e imediatamente confiscado pela censura, Novas cartas portuguesas apresentam uma simultaneidade temporal com o surgimento de movimentos feministas alicerçados, em grande medida, nas questões do corpo e da escrita das mulheres. Exploram-se alguns aspectos do livro à luz dos feminismos de segunda vaga que enformaram os anos 60 e 70 do séc. XX, embora realçando o carácter actual e perforrnativo da escrita de Novas Cartas Portuguesas na construção de outros modelos não dicotómic...

  7. Nova in Centaurus - ASASSN-17gk

    Science.gov (United States)

    Waagen, Elizabeth O.

    2017-05-01

    AAVSO Alert Notice 578 announces the discovery of a galactic nova in Centaurus - ASASSN-17gk - by the ASAS-SN team at magnitude 10.9 V on 2017 May 17.28 UT. Spectroscopy indicating that ASASSN-17gk is a galactic nova was obtained by P. Luckas (International Centre for Radio Astronomy Research, Univ. Western Australia) on 2017 May 18.0598 UT (ATel #10399). Finder charts with sequence may be created using the AAVSO Variable Star Plotter (https://www.aavso.org/vsp). Observations should be submitted to the AAVSO International Database. See full Alert Notice for more details.

  8. The peculiar nova V1309 Sco/Nova Sco 2008: A candidate twin of V838 Mon

    CERN Document Server

    Mason, Elena; Williams, Robert E; Preston, George; Bensby, Thomas

    2010-01-01

    Nova Scorpii 2008 was the target of our Directory Discretionary Time proposal at VLT+UVES in order to study the evolution, origin and abundances of the heavy-element absorption system recently discovered in 80% of classical novae in outburst. The early decline of Nova Scorpii 2008 was monitored with high resolution echelle spectroscopy at 5 different epochs. The analysis of the absorption and the emission lines show many unusual characteristics. Nova Scorpii 2008 is confirmed to differ from a common Classical Nova as well as a Symbiotic Recurrent Nova, and it shows characteristics which are common to the so called, yet debated, red-novae. The origin of this new nova remains uncertain.

  9. Qualidade da carne de cordeiros Santa Inês terminados com diferentes dietas Quality of Santa Ines lamb meat terminated with different diets

    Directory of Open Access Journals (Sweden)

    Marta Suely Madruga

    2005-02-01

    Full Text Available Foram avaliados os aspectos qualitativos da carne de cordeiros Santa Inês submetidos, na fase de terminação, a sistemas de alimentação diferenciados. Foram analisadas 24 pernas de cordeiros não-castrados, com idade de abate entre seis e dez meses, distribuídos eqüitativamente segundo as dietas recebidas: T1 = feno de capim-d'água + concentrado, T2 = feno de restolho de abacaxi + concentrado, T3 = palma + mistura, T4 = silagem de milho + concentrado. A utilização de quatro tipos de alimentos volumosos exerceu influência significativa sobre os teores de composição centesimal, cálcio, fósforo, colesterol, fosfolipídios, ácidos graxos saturados e poliinsaturados e nos parâmetros sensoriais da carne de ovinos Santa Inês. Os cordeiros alimentados com volumosos energéticos (T1, T2 e T4 apresentaram carnes com maiores concentrações lipídicas em (6,93; 8,09 e 8,38%, respectivamente, melhor qualidade sensorial e maiores percentuais de ácidos graxos monoinsaturados (C18:1, C16:1, com médias de 41,38; 46,40; 43,15 e 3,44; 3,34; e 2,76%, respectivamente. O uso de palma forrageira (T3 na alimentação dos cordeiros resultou em uma carne com teores de umidade, proteínas, fósforo, cálcio, colesterol e ácidos graxos saturados significativamente maiores em relação aos demais volumosos (T1, T2 e T4, porém com qualidade sensorial inferior.This study had the objective of evaluating the qualitative aspects of lamb meat from Santa Ines breed when submitted in the termination phase to different feeding systems. Twenty four legs from entire lambs with slaughter age from six to ten months were equally distributed among four different diets: T1 = capim-d'água hay + concentrate, T2 = pineapple hay + concentrate, T3 = forage palm + mixture, T4 = maize ensilage hay + concentrate. The utilization of four different forager feeds resulted in significant difference among the percentages of centesimal composition, calcium, phosphorus, cholesterol

  10. Desempenho e características de carcaças de cordeiros suplementados com diferentes níveis de resíduo de biodiesel

    Directory of Open Access Journals (Sweden)

    B.C. Soares

    2012-12-01

    Full Text Available Estudou-se a suplementação de dietas de cordeiros confinados com resíduo de biodiesel, utilizando-se 25 ovinos, SRD, machos, castrados, com média de peso de 20kg. O delineamento experimental foi de blocos ao acaso, com cinco repetições por tratamento e esquema de parcelas subdivididas para os dados de biometria. O experimento teve a duração de 70 dias. As dietas eram compostas de 34% de volumoso e 61% de concentrado, à base de milho, soja, minerais e 5% de óleo de dendê ou resíduo de biodiesel, em percentagens crescentes - zero, 25, 50, 75 e 100%. Os animais foram abatidos ao final do experimento para avaliação da carcaça. Foram observados efeitos significativos (P<0,05 de percentagem de inclusão do resíduo, para as variáveis de desempenho e biometria demonstrados nos efeitos lineares crescentes das equações de regressão, assim como para peso da carcaça quente (PCQ -, com médias de 14; 15,92; 16,14; 16,42 e 18,02% - e peso da carcaça fria (PCF -, com médias de 13,12; 14,78; 15,06; 15,70 e 17,25% -, para dietas com, respectivamente, 0, 25, 50, 100% de resíduo de biodiesel de dendê. A utilização de resíduo de biodiesel de dendê na alimentação de cordeiros em crescimento é alternativa para aumentar a densidade energética de suas dietas.

  11. Condição hepática de cordeiros mantidos com dietas contendo torta de dendê proveniente da produção de biodiesel

    OpenAIRE

    Nunes, Alexandro Silva; Oliveira, Ronaldo Lopes; Ayres, Maria Consuêlo Caribé; Bagaldo, Adriana Regina; Garcez Neto,Américo Fróes; Barbosa,Larissa Pires

    2010-01-01

    P. 1825-1831. Esta pesquisa foi conduzida com o objetivo de verificar o melhor nível de torta de dendê na dieta de cordeiros por meio da avaliação da condição hepática. Foram utilizados 32 cordeiros Santa Inês não-castrados distribuídos em quatro dietas com 0,0; 6,5; 13,0 e 19,5% de torta de dendê na matéria seca (MS). A cada 15 dias, foram coletadas amostras de sangue dos animais, totalizando cinco coletas em todo o período experimental. Foram determinados os teores de triglicérides, cole...

  12. Condição hepática de cordeiros mantidos com dietas contendo torta de dendê proveniente da produção de biodiesel

    OpenAIRE

    Nunes, Alexandro Silva; Oliveira, Ronaldo Lopes; Ayres,Maria Consuelo Caribe; Bagaldo, Adriana Regina; Garcez Neto,Américo Fróes; Barbosa,Larissa Pires

    2010-01-01

    Esta pesquisa foi conduzida com o objetivo de verificar o melhor nível de torta de dendê na dieta de cordeiros por meio da avaliação da condição hepática. Foram utilizados 32 cordeiros Santa Inês não-castrados distribuídos em quatro dietas com 0,0; 6,5; 13,0 e 19,5% de torta de dendê na matéria seca (MS). A cada 15 dias, foram coletadas amostras de sangue dos animais, totalizando cinco coletas em todo o período experimental. Foram determinados os teores de triglicérides, colesterol, proteínas...

  13. Pre-nova X-ray observations of V2491 Cyg (Nova Cyg 2008b)

    CERN Document Server

    Ibarra, A; Osborne, J P; Page, K; Ness, J U; Saxton, R D; Baumgartner, W; Beckmann, V; Bode, M F; Hernanz, M; Mukai, K; Orio, M; Sala, G; Starrfield, S; Wynn, G A

    2009-01-01

    Classical novae are phenomena caused by explosive hydrogen burning on an accreting white dwarf. So far, only one classical nova has been identified in X-rays before the actual optical outburst occurred (V2487 Oph). The recently discovered nova, V2491 Cyg, is one of the fastest (He/N) novae observed so far. Using archival ROSAT, XMM-Newton and Swift data, we show that V2491 Cyg was a persistent X-ray source during its quiescent time before the optical outburst. We present the X-ray spectral characteristics and derive X-ray fluxes. The pre-outburst X-ray emission is variable, and at least in one observation it shows a very soft X-ray source.

  14. NOVA Making Stuff Season 2

    Energy Technology Data Exchange (ETDEWEB)

    Leombruni, Lisa; Paulsen, Christine Andrews

    2014-12-12

    Over the course of four weeks in fall 2013, 11.7 million Americans tuned in to PBS to follow host David Pogue as he led them in search of engineering and scientific breakthroughs poised to change our world. Levitating trains, quantum computers, robotic bees, and bomb-detecting plants—these were just a few of the cutting-edge innovations brought into the living rooms of families across the country in NOVA’s four-part series, Making Stuff: Faster, Wilder, Colder, and Safer. Each of the four one-hour programs gave viewers a behind-the-scenes look at novel technologies poised to change our world—showing them how basic research and scientific discovery can hold the keys to transforming how we live. Making Stuff Season 2 (MS2) combined true entertainment with educational value, creating a popular and engaging series that brought accessible science into the homes of millions. NOVA’s goal to engage the public with such technological innovation and basic research extended beyond the broadcast series, including a variety of online, educational, and promotional activities: original online science reporting, web-only short-form videos, a new online quiz-game, social media engagement and promotion, an educational outreach “toolkit” for science educators to create their own “makerspaces,” an online community of practice, a series of nationwide Innovation Cafés, educator professional development, a suite of teacher resources, an “Idealab,” participation in national conferences, and specialized station relation and marketing. A summative evaluation of the MS2 project indicates that overall, these activities helped make a significant impact on the viewers, users, and participants that NOVA reached. The final evaluation conducted by Concord Evaluation Group (CEG) confidently concluded that the broadcast, website, and outreach activities were successful at achieving the project’s intended impacts. CEG reported that the MS2 series and website content were

  15. NOVA making stuff: Season 2

    Energy Technology Data Exchange (ETDEWEB)

    Leombruni, Lisa [WGBH Educational Foundation, Boston, MA (United States); Paulsen, Christine Andrews [Concord Evaluation Group, Concord, MA (United States)

    2014-12-12

    Over the course of four weeks in fall 2013, 11.7 million Americans tuned in to PBS to follow host David Pogue as he led them in search of engineering and scientific breakthroughs poised to change our world. Levitating trains, quantum computers, robotic bees, and bomb-detecting plants—these were just a few of the cutting-edge innovations brought into the living rooms of families across the country in NOVA’s four-part series, Making Stuff: Faster, Wilder, Colder, and Safer. Each of the four one-hour programs gave viewers a behind-the-scenes look at novel technologies poised to change our world—showing them how basic research and scientific discovery can hold the keys to transforming how we live. Making Stuff Season 2 (MS2) combined true entertainment with educational value, creating a popular and engaging series that brought accessible science into the homes of millions. NOVA’s goal to engage the public with such technological innovation and basic research extended beyond the broadcast series, including a variety of online, educational, and promotional activities: original online science reporting, web-only short-form videos, a new online quiz-game, social media engagement and promotion, an educational outreach “toolkit” for science educators to create their own “makerspaces,” an online community of practice, a series of nationwide Innovation Cafés, educator professional development, a suite of teacher resources, an “Idealab,” participation in national conferences, and specialized station relation and marketing. A summative evaluation of the MS2 project indicates that overall, these activities helped make a significant impact on the viewers, users, and participants that NOVA reached. The final evaluation conducted by Concord Evaluation Group (CEG) confidently concluded that the broadcast, website, and outreach activities were successful at achieving the project’s intended impacts. CEG reported that the MS2 series and website content were

  16. Desenvolvimento corporal e relação entre biometria e peso de cordeiros lactantes da raça Santa Inês criados na Amazônia

    Directory of Open Access Journals (Sweden)

    D.S. Souza

    2014-12-01

    Full Text Available Objetivou-se com este trabalho descrever as medidas biométricas de cordeiros lactantes da raça Santa Inês criados em condições amazônicas; estabelecer relação entre a idade e as medidas corporais; bem como correlacionar essas medidas biométricas com o peso corporal. Utilizaram-se 75 animais criados em sistema semi-intensivo, submetidos a mensurações do peso corporal (PC, comprimento corporal (CC, altura do anterior (AA e do posterior (AP, perímetro torácico (PT, largura da garupa (LG e do peito (LP, comprimento da perna (CP, perímetro da perna (PP e compacidade corporal (COMPC, ao nascer e aos 15, 30, 45 e 60 dias de idade. Somente as medidas LG e PP demonstraram regressões com R2 abaixo de 0,70 em relação à idade dos cordeiros. Todas as medidas corporais utilizadas nesta pesquisa, individualmente, demonstraram r positivo com o peso corporal. As variáveis biométricas que melhor compuseram a equação de predição do peso dos cordeiros utilizados neste estudo foram CC, AP, PT, LG e PP. Concluiu-se que a idade de cordeiros pode ser utilizada como preditora do peso e de algumas medidas biométricas corporais e que o peso pode ser estimado por meio de algumas medidas biométricas.

  17. ULF fluctuations at Terra Nova Bay (Antarctica

    Directory of Open Access Journals (Sweden)

    A. Meloni

    2000-06-01

    Full Text Available ULF geomagnetic field measurements in Antarctica are a very important tool for better understanding the dynamics of the Earth’s magnetosphere and its response to the variable solar wind conditions. We review the results obtained in the last few years at the Italian observatory at Terra Nova Bay

  18. When does an old nova become a dwarf nova? Kinematics and age of the nova shell of the dwarf nova AT Cnc

    CERN Document Server

    Shara, Michael M; Martin, Thomas; Alarie, Alexandre

    2016-01-01

    The Z Cam-type dwarf nova AT Cnc displays a classical nova (CN) shell, demonstrating that mass transfer in cataclysmic binaries decreases substantially after a CN eruption. The hibernation scenario of cataclysmic binaries predicts such a decrease, on a timescale of a few centuries. In order to measure the time since AT Cnc's last CN eruption, we have measured the radial velocities of a hundred clumps in its ejecta with SITELLE, CFHT's recently commissioned imaging Fourier transform spectrometer. These range from -455 to +490 km/s. Coupled with the known distance to AT Cnc of 460 pc (Shara 2012), the size of AT Cnc's shell, and a simple model of nova ejecta deceleration, we determine that the last CN eruption of this system occurred $330_{-90}^{+135}$ years ago. This is the most rapid transition from a high mass transfer rate, novalike variable to a low mass transfer rate, dwarf nova yet measured, and in accord with the hibernation scenario of cataclysmic binaries. We conclude by noting the similarity in deduc...

  19. The expanding fireball of Nova Delphini 2013.

    Science.gov (United States)

    Schaefer, G H; ten Brummelaar, T; Gies, D R; Farrington, C D; Kloppenborg, B; Chesneau, O; Monnier, J D; Ridgway, S T; Scott, N; Tallon-Bosc, I; McAlister, H A; Boyajian, T; Maestro, V; Mourard, D; Meilland, A; Nardetto, N; Stee, P; Sturmann, J; Vargas, N; Baron, F; Ireland, M; Baines, E K; Che, X; Jones, J; Richardson, N D; Roettenbacher, R M; Sturmann, L; Turner, N H; Tuthill, P; van Belle, G; von Braun, K; Zavala, R T; Banerjee, D P K; Ashok, N M; Joshi, V; Becker, J; Muirhead, P S

    2014-11-13

    A classical nova occurs when material accreting onto the surface of a white dwarf in a close binary system ignites in a thermonuclear runaway. Complex structures observed in the ejecta at late stages could result from interactions with the companion during the common-envelope phase. Alternatively, the explosion could be intrinsically bipolar, resulting from a localized ignition on the surface of the white dwarf or as a consequence of rotational distortion. Studying the structure of novae during the earliest phases is challenging because of the high spatial resolution needed to measure their small sizes. Here we report near-infrared interferometric measurements of the angular size of Nova Delphini 2013, starting one day after the explosion and continuing with extensive time coverage during the first 43 days. Changes in the apparent expansion rate can be explained by an explosion model consisting of an optically thick core surrounded by a diffuse envelope. The optical depth of the ejected material changes as it expands. We detect an ellipticity in the light distribution, suggesting a prolate or bipolar structure that develops as early as the second day. Combining the angular expansion rate with radial velocity measurements, we derive a geometric distance to the nova of 4.54 ± 0.59 kiloparsecs from the Sun.

  20. Cinema Interativo: novas possibilidades de ambientes imersivos

    Directory of Open Access Journals (Sweden)

    Natália Aly Menezes

    2011-12-01

    Full Text Available O texto “Cinema Interativo: novas possibilidades de ambientes imersivos”, sintetiza a pesquisa  de-senvolvida pela autora, como projeto de Pós-Graduação no curso Tecnologia da Inteligência e Design Digital – PUC-SP. A pesquisa busca reunir uma análise atenciosa diante da entrada da tecnologia di-gital, tecnologia esta que interfere inevitavelmente na linguagem cinematográfica, e não apenas em sua estética. Com a abertura do mundo dos números binários (código das informações computacionais, e a possibilidade de digitalização da imagem, o que era matéria se desmaterializa e infinitas possibilidades criacionais surgem, inclusive, abrindo portas para experimentar o cinema de maneira expandida. No-vas formas de construção narrativa, nova relação espectador-cinema, um novo tempo e espaço, novas formas de significações; tudo pode sofrer alterações. O texto parte de estudos feitos com base em teóri-cos como Peter Weibel, Jeffrey Shaw, Lev Manovich, entre outros.

  1. Modos de vida alternativos: o caso da comunidade Noiva do Cordeiro http://dx.doi.org/10.15601/1983-7631/rt.v3n5p152-158

    Directory of Open Access Journals (Sweden)

    Adilson Schultz

    2011-04-01

    Full Text Available Noiva do cordeiro é uma comunidade rural liderada por mulheres, que desenvolveu um modo de vida alternativo e sustentável, com partilha de bens e fim da religião institucionalizada. Forjado ao longo de mais de um século, num processo de constantes rupturas religiosas, familiares e ideológicas, esse inusitado modo de vida produziu uma comunidade autônoma, com sujeitos autônomos e responsáveis uns pelos outros, que se tornaram lideranças sociais e políticas. No centro de sua história, experiências de sofrimento e rupturas relacionadas à religião, à fome, e à estrutura familiar patriarcal. O estudo do caso de Noiva do Cordeiro tem a intenção de analisar elementos subjetivos deste processo, verificando os indicativos e as implicações de tal fenômeno religioso e social, especialmente os limites e o fim de determinado modelo de religião. Os pressupostos teóricos deste estudo apontam para uma perspectiva transdisciplinar que compreende a teologia, a sociologia e a psicologia da religião e, nestes campos, as teorias feministas.Palavras-chave: Noiva do Cordeiro; modos de vida alternativos; fim da religião; liderança de mulheres; valores humanos

  2. The NOvA software testing framework

    Science.gov (United States)

    Tamsett, M.; C Group

    2015-12-01

    The NOvA experiment at Fermilab is a long-baseline neutrino experiment designed to study vε appearance in a vμ beam. NOvA has already produced more than one million Monte Carlo and detector generated files amounting to more than 1 PB in size. This data is divided between a number of parallel streams such as far and near detector beam spills, cosmic ray backgrounds, a number of data-driven triggers and over 20 different Monte Carlo configurations. Each of these data streams must be processed through the appropriate steps of the rapidly evolving, multi-tiered, interdependent NOvA software framework. In total there are greater than 12 individual software tiers, each of which performs a different function and can be configured differently depending on the input stream. In order to regularly test and validate that all of these software stages are working correctly NOvA has designed a powerful, modular testing framework that enables detailed validation and benchmarking to be performed in a fast, efficient and accessible way with minimal expert knowledge. The core of this system is a novel series of python modules which wrap, monitor and handle the underlying C++ software framework and then report the results to a slick front-end web-based interface. This interface utilises modern, cross-platform, visualisation libraries to render the test results in a meaningful way. They are fast and flexible, allowing for the easy addition of new tests and datasets. In total upwards of 14 individual streams are regularly tested amounting to over 70 individual software processes, producing over 25 GB of output files. The rigour enforced through this flexible testing framework enables NOvA to rapidly verify configurations, results and software and thus ensure that data is available for physics analysis in a timely and robust manner.

  3. Terra Nova development : challenges and lessons learned

    Energy Technology Data Exchange (ETDEWEB)

    Lever, G. [Petro-Canada, Inc. (Canada)

    2001-07-01

    The major oil and gas fields in Canada's east coast were illustrated for this power point presentation which focused on the development concept of the Terra Nova. Terra Nova is the first floating production system (FPSO) development and only the second offshore oil development on the challenging Grand Banks of Newfoundland. It is also the first offshore facility in Canada to be certified to both offshore petroleum and shipping regulations. In addition, it represents the first fully-automated disconnectable turret, riser and mooring system on an FPSO, and the first to have glory holes for protecting subsea equipment from iceberg damage. The FPSO can withstand an impact with a 100,000 tonne iceberg. The Terra Nova project also represents the first attempt at trenching in stiff hard pan soil conditions which are typical of the Grand Banks. The physical environment design criteria for the Terra Nova in terms of water depth, air temperature, water temperature, icebergs, current, wind and waves were provided along with the functional requirements in terms of oil production, gas compression, total fluids, water injection, produced water, gas injection and water injection. An illustration of the FPSO topsides modules layout was also provided. The alliance-based contracting approach was adopted in 1995 and gave Petro-Canada access to the collective capability of major contractors that were able to face the technical challenges on Terra Nova. Some of the lessons learned from this contracting approach are that a strong central technical integration team should be implemented early and maintained through to project completion and that interfaces must be identified early and managed in a manner according to risk associated with the cost and schedule. tabs., figs.

  4. Comportamento ingestivo de cordeiros alimentados com torta de macaúba Ingestive behavior of lambs fed with macauba meal

    Directory of Open Access Journals (Sweden)

    R.A. Azevedo

    2013-04-01

    Full Text Available Avaliaram-se os efeitos de diferentes porcentagens (0, 10, 20 e 30% de inclusão da torta de macaúba (TM no comportamento ingestivo de 24 cordeiros Santa Inês, com média de cinco meses de idade e peso vivo de 23,9kg, distribuídos em delineamento em blocos ao acaso, com quatro tratamentos e seis repetições, durante 60 dias de confinamento. Foram avaliados os tempos médios despendidos com alimentação, ruminação (TR, ócio (TO, tempo de mastigação total (TMT, eficiência de alimentação (EA MS e EA FDN e eficiência de ruminação, além do número de bolos ruminados (NBR e número diário de mastigações merícicas (MMnd. A adição de TM à dieta aumentou linearmente o TR, TMT, NBR, MMnd e EA FDN e reduziu de forma linear o TO, em consequência do maior teor de fibra em detergente neutro das dietas com o coproduto. Mesmo com o aumento no TMT, não foi verificada diferença no consumo e na eficiência de ruminação e alimentação da matéria seca, possivelmente em razão da baixa efetividade de fibra da TM, demonstrando o potencial de utilização desse coproduto na dieta de ovinos em crescimento.The effects of different percentages (0, 10, 20 and 30% of inclusion of macauba meal (MM on the ingestive behavior of 24 Santa Inês male lambs, averaging five months of age and 23.9kg of initial body weight were studied. The animals were allotted to a completely randomized block design with four treatments and six replications during 60 days of confinement. The variables measured were time spent in rumination (TR, idle time (IT, total chewing (TC, power efficiency (PE DM and PE NDF and efficiency of rumination, as well as the number of ruminated bolus (NRB and daily number of chews (Cnd. The addition of MM to the diet increased TR, TC, NRB, Cnb and PE NDF linearly, and reduced IT linearly, as a result of higher content of neutral detergent fiber in the diet. Although there was an increase in TC, no difference was verified in the

  5. The awakening of a classical nova from hibernation

    Science.gov (United States)

    Mróz, Przemek; Udalski, Andrzej; Pietrukowicz, Paweł; Szymański, Michał K.; Soszyński, Igor; Wyrzykowski, Łukasz; Poleski, Radosław; Kozłowski, Szymon; Skowron, Jan; Ulaczyk, Krzysztof; Skowron, Dorota; Pawlak, Michał

    2016-09-01

    Cataclysmic variable stars—novae, dwarf novae, and nova-likes—are close binary systems consisting of a white dwarf star (the primary) that is accreting matter from a low-mass companion star (the secondary). From time to time such systems undergo large-amplitude brightenings. The most spectacular eruptions, with a ten-thousandfold increase in brightness, occur in classical novae and are caused by a thermonuclear runaway on the surface of the white dwarf. Such eruptions are thought to recur on timescales of ten thousand to a million years. In between, the system’s properties depend primarily on the mass-transfer rate: if it is lower than a billionth of a solar mass per year, the accretion becomes unstable and the matter is dumped onto the white dwarf during quasi-periodic dwarf nova outbursts. The hibernation hypothesis predicts that nova eruptions strongly affect the mass-transfer rate in the binary, keeping it high for centuries after the event. Subsequently, the mass-transfer rate should significantly decrease for a thousand to a million years, starting the hibernation phase. After that the nova awakes again—with accretion returning to the pre-eruption level and leading to a new nova explosion. The hibernation model predicts cyclical evolution of cataclysmic variables through phases of high and low mass-transfer. The theory gained some support from the discovery of ancient nova shells around the dwarf novae Z Camelopardalis and AT Cancri, but direct evidence for considerable mass-transfer changes prior, during and after nova eruptions has not hitherto been found. Here we report long-term observations of the classical nova V1213 Cen (Nova Centauri 2009) covering its pre- and post-eruption phases and precisely documenting its evolution. Within the six years before the explosion, the system revealed dwarf nova outbursts indicative of a low mass-transfer rate. The post-nova is two orders of magnitude brighter than the pre-nova at minimum light with no trace of

  6. The awakening of a classical nova from hibernation.

    Science.gov (United States)

    Mróz, Przemek; Udalski, Andrzej; Pietrukowicz, Paweł; Szymański, Michał K; Soszyński, Igor; Wyrzykowski, Łukasz; Poleski, Radosław; Kozłowski, Szymon; Skowron, Jan; Ulaczyk, Krzysztof; Skowron, Dorota; Pawlak, Michał

    2016-09-29

    Cataclysmic variable stars-novae, dwarf novae, and nova-likes-are close binary systems consisting of a white dwarf star (the primary) that is accreting matter from a low-mass companion star (the secondary). From time to time such systems undergo large-amplitude brightenings. The most spectacular eruptions, with a ten-thousandfold increase in brightness, occur in classical novae and are caused by a thermonuclear runaway on the surface of the white dwarf. Such eruptions are thought to recur on timescales of ten thousand to a million years. In between, the system's properties depend primarily on the mass-transfer rate: if it is lower than a billionth of a solar mass per year, the accretion becomes unstable and the matter is dumped onto the white dwarf during quasi-periodic dwarf nova outbursts. The hibernation hypothesis predicts that nova eruptions strongly affect the mass-transfer rate in the binary, keeping it high for centuries after the event. Subsequently, the mass-transfer rate should significantly decrease for a thousand to a million years, starting the hibernation phase. After that the nova awakes again-with accretion returning to the pre-eruption level and leading to a new nova explosion. The hibernation model predicts cyclical evolution of cataclysmic variables through phases of high and low mass-transfer. The theory gained some support from the discovery of ancient nova shells around the dwarf novae Z Camelopardalis and AT Cancri, but direct evidence for considerable mass-transfer changes prior, during and after nova eruptions has not hitherto been found. Here we report long-term observations of the classical nova V1213 Cen (Nova Centauri 2009) covering its pre- and post-eruption phases and precisely documenting its evolution. Within the six years before the explosion, the system revealed dwarf nova outbursts indicative of a low mass-transfer rate. The post-nova is two orders of magnitude brighter than the pre-nova at minimum light with no trace of dwarf

  7. Características quantitativas da carcaça de cordeiros de diferentes genótipos submetidos a duas dietas Quantitative traits of carcass from lambs of different genotypes submitted to two diets

    Directory of Open Access Journals (Sweden)

    Felipe Queiroga Cartaxo

    2011-10-01

    Full Text Available Objetivou-se avaliar as características quantitativas de carcaça de cordeiros de diferentes genótipos recebendo diversos níveis de energia na dieta. Foram utilizados 54 cordeiros não-castrados, sendo 18 Santa Inês (SI, 18 F1Dorper × Santa Inês (Dp × SI e 18 F1 Santa Inês × Sem Raça Definida (SI × SRD, com idade média de 150 dias e peso médio de 22,60 kg no início do experimento. As dietas continham 17% de proteína bruta e 2,40 Mcal/kg MS ou 2,90 Mcal/kg MS. Os cordeiros alimentados com a dieta contendo 2,90 Mcal/kg MS apresentaram maior peso corporal e de carcaça, área de olho-de-lombo, percentual de gordura interna, índice de musculosidade, índice de compacidade da carcaça, percentual de gordura e menor relação músculo:gordura. As carcaças desses cordeiros obtiveram também menores perdas por resfriamento e maior peso e percentual de paleta e perna. As carcaças dos cordeiros Dorper × Santa Inês foram superiores em espessura de gordura subcutânea, medida GR (gordura sobre a 12ª costela a 11 cm de distância da linha média lombo, percentual de gordura, relação músculo:osso, índice de musculosidade, peso e percentual de lombo. Os cordeiros Santa Inês apresentaram maior relação músculo:gordura. A dieta e o genótipo influenciam as características quantitativas de carcaça de cordeiros.The objective of this study was to evaluate the quantitative carcass traits of lambs from different genotypes receiving different levels of energy in the diet. Fifty-four non-castrated lambs - 18 Santa Inês (SI, 18 F1Dorper × Santa Inês (Dp × SI and 18 F1Santa Inês × No defined breed (SI × NDB - of average 150 days old and 22.6-kg BW were used in the beginning of the experiment. Diets contained 17% crude protein and 2.40 Mcal/kg DM or 2.90 Mcal/kg DM. Lambs fed the diet containing 2.90 Mcal/kg DM showed higher final live and carcass weight, loin eye area, percentage of internal fat, muscularity index, compactness of the

  8. Dwarf Nova Outbursts with Magnetorotational Turbulence

    CERN Document Server

    Coleman, M S B; Blaes, O; Lasota, J -P; Hirose, S

    2016-01-01

    The phenomenological Disc Instability Model has been successful in reproducing the observed light curves of dwarf nova outbursts by invoking an enhanced Shakura-Sunyaev $\\alpha$ parameter $\\sim0.1-0.2$ in outburst compared to a low value $\\sim0.01$ in quiescence. Recent thermodynamically consistent simulations of magnetorotational (MRI) turbulence with appropriate opacities and equation of state for dwarf nova accretion discs have found that thermal convection enhances $\\alpha$ in discs in outburst, but only near the hydrogen ionization transition. At higher temperatures, convection no longer exists and $\\alpha$ returns to the low value comparable to that in quiescence. In order to check whether this enhancement near the hydrogen ionization transition is sufficient to reproduce observed light curves, we incorporate this MRI-based variation in $\\alpha$ into the Disc Instability Model, as well as simulation-based models of turbulent dissipation and convective transport. These MRI-based models can successfully r...

  9. Tycho Brahe and the Nova of 1572

    Science.gov (United States)

    Gingerich, O.

    2005-12-01

    The brilliant Nova of 1572 marked the beginning of the end of Aristotelian cosmology and provided the defining moment when the young Tycho Brahe became a professional astronomer. He received more than a ton of gold from the Danish king to build his Uraniborg Observatory. His instruments, the finest produced in the pre-telescopic age, enabled him to establish that both the nova and the Comet of 1577 lay beyond the moon, contrary to Aristotle's teaching. His major attempt to establish the distance to Mars (in order to distinguish between the Ptolemaic and Copernican cosmologies) failed, but left in its wake a magnificently accurate set of data that enabled Kepler to make the greatest advance in celestial mechanics since Copernicus himself.

  10. Quark Nova Model for Fast Radio Bursts

    CERN Document Server

    Shand, Zachary; Koning, Nico; Ouyed, Rachid

    2015-01-01

    FRBs are puzzling, millisecond, energetic radio transients with no discernible source; observations show no counterparts in other frequency bands. The birth of a quark star from a parent neutron star experiencing a quark nova - previously thought undetectable when born in isolation - provides a natural explanation for the emission characteristics of FRBs. The generation of unstable r-process elements in the quark nova ejecta provides millisecond exponential injection of electrons into the surrounding strong magnetic field at the parent neutron star's light cylinder via $\\beta$-decay. This radio synchrotron emission has a total duration of hundreds of milliseconds and matches the observed spectrum while reducing the inferred dispersion measure by approximately 200 cm$^{-3}$ pc. The model allows indirect measurement of neutron star magnetic fields and periods in addition to providing astronomical measurements of $\\beta$-decay chains of unstable neutron rich nuclei. Using this model, we can calculate expected FR...

  11. Neutrino Oscillation Results from NOvA

    CERN Document Server

    CERN. Geneva

    2016-01-01

    NOvA is an accelerator long-baseline neutrino oscillation experiment optimised to measure electron neutrino appearance in a high-purity beam of muon neutrinos from Fermilab. The exciting discovery of the theta13 neutrino mixing angle in 2012 has opened a door to making multiple new measurements of neutrinos. These include leptonic CP violation, the neutrino mass ordering and the octant of theta23. NOvA with its 810km baseline and higher energy beam has about triple the matter effect of T2K which opens a new window on the neutrino mass ordering. With about 20% of our design beam exposure and significant analysis improvements we have recently released updated results. I will present both our disappearance and appearance measurements.

  12. Discovery of an eclipsing dwarf nova in the ancient nova shell Te 11

    CERN Document Server

    Miszalski, Brent; Littlefair, Stuart P; Warner, Brian; Boffin, Henri M J; Corradi, Romano L M; Jones, David; Motsoaledi, Mokhine; Rodríguez-Gil, Pablo; Sabin, Laurence; Santander-García, Miguel

    2015-01-01

    We report on the discovery of an eclipsing dwarf nova (DN) inside the peculiar, bilobed nebula Te 11. Modelling of high-speed photometry of the eclipse finds the accreting white dwarf to have a mass 1.18 M$_\\odot$ and temperature 13 kK. The donor spectral type of M2.5 results in a distance of 330 pc, colocated with Barnard's loop at the edge of the Orion-Eridanus superbubble. The perplexing morphology and observed bow shock of the slowly-expanding nebula may be explained by strong interactions with the dense interstellar medium in this region. We match the DN to the historic nova of 483 CE in Orion and postulate that the nebula is the remnant of this eruption. This connection supports the millennia time scale of the post-nova transition from high to low mass-transfer rates. Te 11 constitutes an important benchmark system for CV and nova studies as the only eclipsing binary out of just three DNe with nova shells.

  13. The SuperNova Early Warning System

    OpenAIRE

    Scholberg, K.

    2008-01-01

    A core collapse in the Milky Way will produce an enormous burst of neutrinos in detectors world-wide. Such a burst has the potential to provide an early warning of a supernova's appearance. I will describe the nature of the signal, the sensitivity of current detectors, and SNEWS, the SuperNova Early Warning System, a network designed to alert astronomers as soon as possible after the detected neutrino signal.

  14. Nova pulse power system description and status

    Energy Technology Data Exchange (ETDEWEB)

    Holloway, R.W.; Whitham, K.; Merritt, B.T.; Gritton, D.G.; Oicles, J.A.

    1981-06-01

    The Nova laser system is designed to produce critical data in the nation's inertial confinement fusion effort. It is the world's largest peak power laser and presents various unique pulse power problems. In this paper, pulse power systems for this laser are described, the evolutionary points from prior systems are pointed out, and the current status of the hardware is given.

  15. /sup 7/Li production in Nova explosions

    Energy Technology Data Exchange (ETDEWEB)

    Starrfield, S.; Truran, J.W.; Sparks, W.M.; Arnould, M.

    1978-06-01

    Calculations of /sup 7/Li production occurring as a concomitant of thermonuclear runaways in hydrogen envelopes of white dwarfs are reported. It is found that sufficient /sup 7/Li can be produced in models displaying fast--nova-like features to suggest that the corresponding objects represent significant contributors to the /sup 7/Li enrichment of galactic matter. The sensitivities of these results to various assumptions and uncertainties are discussed.

  16. Shocks in nova outflows. I. Thermal emission

    CERN Document Server

    Metzger, Brian D; Vurm, Indrek; Beloborodov, Andrei M; Chomiuk, Laura; Sokoloski, J L; Nelson, Thomas

    2014-01-01

    Evidence for shocks in nova outflows include (1) multiple velocity components in the optical spectra; (2) keV X-ray emission weeks to months after the outburst; (3) early radio flare on timescales of months, in excess of that predicted from the freely expanding photo-ionized gas; and (4) ~ GeV gamma-rays. We present a 1D model for the shock interaction between the fast nova outflow and a dense external shell (DES) and its associated thermal X-ray, optical, and radio emission. The forward shock is radiative initially when the density of shocked gas is highest, at which times radio emission originates from the dense cooling layer immediately downstream of the shock. The radio light curve is characterized by sharper rises to maximum and later peak times at progressively lower frequencies, with a peak brightness temperature that is approximately independent of frequency. We apply our model to the recent gamma-ray classical nova V1324 Sco, obtaining an adequate fit to the early radio maximum for reasonable assumpt...

  17. Introduction to the Nova technical contract

    Energy Technology Data Exchange (ETDEWEB)

    Lindl, J.D.; Kilkenny, J.D.

    1996-06-01

    The 1990 National Academy of Sciences (NAS) final report recommended proceeding with the construction of a 1-to 2-MJ Nd-doped glass laser designed to achieve ignition in the laboratory (a laser originally called the Nova Upgrade, but now called the National Ignition Facility, or NIF, and envisioned as a national user facility). As a prerequisite, the report recommended completion of a series of target physics objectives on the Nova laser in use at the Lawrence Livermore National Laboratory (LLNL). Meeting these objectives, which were called the Nova Technical Contract (NTC), would demonstrate (the Academy committee believed) that the physics of ignition targets was understood well enough that the laser requirements could be accurately specified. Completion of the NTC objectives was given the highest priority (it was Recommendation 1.1) in the NAS report. The NAS committee also recommended a concentrated effort on advanced target design for ignition. As recommended in the report, completion of these objectives has been the joint responsibility of LLNL and the Los Alamos National Laboratory. Most of the articles in this issue of the ICF Quarterly were written jointly by scientists from both institutions. The original NTC objectives have been largely met. This Introduction summarizes those objectives and their motivation in the context of the requirements for ignition.

  18. Dwarf nova outbursts with magnetorotational turbulence

    Science.gov (United States)

    Coleman, M. S. B.; Kotko, I.; Blaes, O.; Lasota, J.-P.; Hirose, S.

    2016-11-01

    The phenomenological disc instability model has been successful in reproducing the observed light curves of dwarf nova outbursts by invoking an enhanced Shakura-Sunyaev α parameter ˜0.1-0.2 in outburst compared to a low value ˜0.01 in quiescence. Recent thermodynamically consistent simulations of magnetorotational instability (MRI) turbulence with appropriate opacities and equation of state for dwarf nova accretion discs have found that thermal convection enhances α in discs in outburst, but only near the hydrogen ionization transition. At higher temperatures, convection no longer exists and α returns to the low value comparable to that in quiescence. In order to check whether this enhancement near the hydrogen ionization transition is sufficient to reproduce observed light curves, we incorporate this MRI-based variation in α into the disc instability model, as well as simulation-based models of turbulent dissipation and convective transport. These MRI-based models can successfully reproduce observed outburst and quiescence durations, as well as outburst amplitudes, albeit with different parameters from the standard disc instability models. The MRI-based model light curves exhibit reflares in the decay from outburst, which are not generally observed in dwarf novae. However, we highlight the problematic aspects of the quiescence physics in the disc instability model and MRI simulations that are responsible for this behaviour.

  19. A Thousand and One Nova Outbursts

    CERN Document Server

    Epchtein, N; Kovetz, A; Prialnik, D

    2006-01-01

    Multicycle nova evolution models have been calculated over the past twenty years, the number being limited by numerical constraints. Here we present a long-term evolution code that enables a continuous calculation through an unlimited number of nova cycles for an unlimited evolution time, even up to (or exceeding) a Hubble time. Starting with two sets of the three independent nova parameters -- the white dwarf mass, the temperature of its isothermal core, and the rate of mass transfer on to it -- we have followed the evolution of two models, with initial masses of 1 and 0.65 solar masses, accretion rates (constant throughout each calculation) of 1e-11 and 1e-9 solar-masses/yr, and relatively high initial temperatures (as they are likely to be at the onset of the outburst phase), through over 1000 and over 3000 cycles, respectively. The results show that although on the short-term consecutive outbursts are almost identical, on the long-term scale the characteristics change. This is mainly due to the changing c...

  20. Crescimento de regiões da carcaça de cordeiros abatidos com diferentes pesos Growth of carcass parts in slaughter lambs with different weights

    Directory of Open Access Journals (Sweden)

    Lisiane Furtado da Silva

    2000-06-01

    Full Text Available O trabalho foi realizado no Setor de Ovinocultura do Departamento de Zootecnia da Universidade Federal de Santa Maria, objetivando determinar o crescimento das principais partes da carcaça e suas proporções em relação ao peso de corpo vazio e peso de carcaça fria de cordeiros abatidos com diferentes pesos. Foram utilizados 22 cordeiros machos inteiros, filhos de carneiros Texel e ovelhas cruzas (Texel x Ideal. Destes, quatro foram abatidos no início do experimento (24 horas após o nascimento, seis ao desmame (45 dias de idade e os remanescentes aos 28 (6 animais ou 33 kg (6 animais. Os cordeiros foram confinados em baias individuais, com suas respectivas mães, até o desmame. A determinação do crescimento dos cortes da carcaça foi realizada através de equações alométricas, utilizando-se o logaritmo do peso de cada região da carcaça, em função do logaritmo do PCF ou PCV. As proporções de quarto, paleta e pescoço, em relação ao PCV, foram semelhantes (P>0,05 nos pesos de abates estudados, no entanto, houve diferença (PThis work was performed at the Ovine Section of Animal Science Department, at Federal University of Santa Maria, Brazil. The purpose of this experiment was to determine the growth of the carcass cuts and percentages in relation to the empty body weight and cold carcass weight of lambs slaughtered at different weights. Twenty-two intact male lambs, sired by Texel males, from crossbreed Texel-Ideal dams were used. Four lambs were slaughtered at the beginning of the experiment (24 hours after birth and three groups of six lambs were slaughtered at weaning and when reaching the weight of 28 and 33kg. The lambs were confined in individual stall together, with their respective mothers until weaning (45 days of age. To study the growth of the different cuts of the carcass, regression equation of the log. of the weight of each part, as a function of the log. of the empty body weight or cold carcass weight were

  1. De uma morada à outra: processos de re-coabitação entre as gerações From one dwelling to another: intergenerational cohabitation processes

    Directory of Open Access Journals (Sweden)

    Clarice Ehlers Peixoto

    2007-12-01

    Full Text Available Desemprego, divórcio, viuvez, filhos que não saem nunca da casa dos pais são as razões que explicam porque, no Brasil, as gerações mais velhas coabitam cada vez mais com as mais jovens. Retornar para a casa familiar, ou ir morar na casa de um(a filho(a introduz uma nova dinâmica na organização doméstica: a reorganização do espaço - abrir, criar lugares para receber o novo(s membro(s; a adaptação das regras, horários e tarefas às necessidades e atividades de cada um, e do grupo em particular. Morar com três ou quatro gerações implica em uma contribuição material e financeira, mas, também, em um suporte moral e afetivo no apoio logístico do cotidiano doméstico. A vida em comum só é possível se existir este circuito de reciprocidades, senão a coabitação pode quebrar a harmonia familiar e tornar-se violenta.Unemployment, divorce, widowhood, children who never leave their parents' house, these are the reasons that explain why the older generations in Brazil cohabit with the younger generations more than before. Returning to one’s parents’ house, or moving to the children's house introduces a new dynamic into the domestic organization: the reorganization of space - the creation of places to receive new family members; the adaptation of rules, schedules and tasks, to the necessities and activities of each member and to the group's in particular. Living with three or four generations implies a material contribution as well as emotional and moral support for the logistics of daily domestic life. Living together is only possible when there is a circuit of reciprocities; otherwise, cohabitation can provoke violent rupture in the family’s harmony.

  2. Bossa Nova: Introducing modularity into the Bossa Nova domain-specific language

    DEFF Research Database (Denmark)

    Lawall, Julia Laetitia; Duschene, Hervé; Muller, Gilles;

    2005-01-01

    Domain-specific languages (DSLs) have been proposed as a solution to ease the development of programs within a program family. Sometimes, however, experience with the use of a DSL reveals the presence of subfamilies within the family targeted by the language. We are then faced with the question...... modular language, Bossa Nova, and assess the language quantitatively and qualitatively....

  3. Nova como sistema operativo embebido para hardware cubano Nova as embedded operating system for cuban hardware

    Directory of Open Access Journals (Sweden)

    José Ernesto Torres Sánchez

    2012-05-01

    Full Text Available Este trabajo expone los resultados de construir un sistema operativo embebido basado en Nova, el cual brinda las funcionalidades necesarias para crear el Cliente Ligero Cubano, utilizando como componente de hardware, la Computadora en una Tarjeta CID 300/9 diseñada por el Instituto Central de Investigación Digital. Obteniéndose la primera versión de Nova para la arquitectura de computadora Advanced RISC Machine y el primer sistema operativo base, estable y de propósito general para la CID 300/9. Se expone un estado del arte de los sistemas operativos embebidos más utilizados actualmente; la estructura de la solución, los métodos y herramientas empleados para obtenerla.This paper presents the results of the construction a an embedded operating system based on Nova, which provides the needed features to create the Cuban Thin Client, using as hardware component the Computer on a CID 300/9 Board designed by the Central Institute for Digital Research, obtaining the first version of Nova for the Advance RISC Machine  computer architecture and the first base operating system, stable and for general purposes for the CID 300/9. A state of the art of the currently most used embedded operating systems, the solution's structure, the methods and tools used for its development are presented.

  4. Nova as embedded operating system for cuban hardware Nova como sistema operativo embebido para hardware cubano

    Directory of Open Access Journals (Sweden)

    Mijail Hurtado Fedorovich

    2012-05-01

    Full Text Available This paper presents the results of the construction a an embedded operating system based on Nova, which provides the needed features to create the Cuban Thin Client, using as hardware component the Computer on a CID 300/9 Board designed by the Central Institute for Digital Research, obtaining the first version of Nova for the Advance RISC Machine  computer architecture and the first base operating system, stable and for general purposes for the CID 300/9. A state of the art of the currently most used embedded operating systems, the solution's structure, the methods and tools used for its development are presented. Este trabajo expone los resultados de construir un sistema operativo embebido basado en Nova, el cual brinda las funcionalidades necesarias para crear el Cliente Ligero Cubano, utilizando como componente de hardware, la Computadora en una Tarjeta CID 300/9 diseñada por el Instituto Central de Investigación Digital. Obteniéndose la primera versión de Nova para la arquitectura de computadora Advanced RISC Machine y el primer sistema operativo base, estable y de propósito general para la CID 300/9. Se expone un estado del arte de los sistemas operativos embebidos más utilizados actualmente; la estructura de la solución, los métodos y herramientas empleados para obtenerla.

  5. Explosive lithium production in the classical nova V339 Del (Nova Delphini 2013)

    CERN Document Server

    Tajitsu, Akito; Naito, Hiroyuki; Arai, Akir; Aoki, Wako

    2015-01-01

    The origin of lithium (Li) and its production process have long been an unsettled question in cosmology and astrophysics. Candidates environments of Li production events or sites suggested by previous studies include big bang nucleosynthesis, interactions of energetic cosmic rays with interstellar matter, evolved low mass stars, novae, and supernova explosions. Chemical evolution models and observed stellar Li abundances suggest that at least half of the present Li abundance may have been produced in red giants, asymptotic giant branch (AGB) stars, and novae. However, no direct evidence for the supply of Li from stellar objects to the Galactic medium has yet been found. Here we report on the detection of highly blue-shifted resonance lines of the singly ionized radioactive isotope of beryllium, $^{7}$Be, in the near ultraviolet (UV) spectra of the classical nova V339 Del (Nova Delphini 2013). Spectra were obtained 38 to 48 days after the explosion. $^{7}$Be decays to form $^{7}$Li within a short time (half-li...

  6. V4743 Sgr, a magnetic nova?

    Science.gov (United States)

    Zemko, P.; Orio, M.; Mukai, K.; Bianchini, A.; Ciroi, S.; Cracco, V.

    2016-08-01

    Two XMM-Newton observations of Nova V4743 Sgr (Nova Sgr 2002) were performed shortly after it returned to quiescence, 2 and 3.5 yr after the explosion. The X-ray light curves revealed a modulation with a frequency of ≃0.75 mHz, indicating that V4743 Sgr is most probably an intermediate polar (IP). The X-ray spectra have characteristics in common with known IPs, with a hard thermal plasma component that can be fitted only assuming a partially covering absorber. In 2004, the X-ray spectrum had also a supersoft blackbody-like component, whose temperature was close to that of the white dwarf (WD) in the supersoft X-ray phase following the outburst, but with flux by at least two orders of magnitude lower. In quiescent IPs, a soft X-ray flux component originates at times in the polar regions irradiated by an accretion column, but the supersoft component of V4743 Sgr disappeared in 2006, indicating a possible origin different from accretion. We suggest that it may have been due to an atmospheric temperature gradient on the WD surface, or to continuing localized thermonuclear burning at the bottom of the envelope, before complete turn-off. An optical spectrum obtained with Southern African Large Telescope (SALT) 11.5 yr after the outburst showed a prominent He II λ4686 line and the Bowen blend, which reveal a very hot region, but with peak temperature shifted to the ultraviolet range. V4743 Sgr is the third post-outburst nova and IP candidate showing a low-luminosity supersoft component in the X-ray flux a few years after the outburst.

  7. ECONOMIA SOCIAL INCORPORATIVA (e as novas linguagens

    Directory of Open Access Journals (Sweden)

    Welinton dos Santos

    2017-05-01

    Full Text Available A inovação tecnológica aliada à interação de comunicação sem limites, chamada de “Economia Social Incorporativa”, sendo uma rede integrada e sociável as populações do mundo. Baseada em uma pesquisa bibliográfica de caráter qualitativo e documental mostrando que a comunicação, informações e tecnologias evoluem surgindo novos materiais em destaque o grafeno, composto por átomos de carbono com alta condutividade térmica e elétrica, flexível e resistente, material que pode substituir o silício e permitir a segunda revolução tecnológica e levando consigo a economia. Com esses feitos tecnológicos a humanidade tende a estar mais do que nunca com uma ligação inseparável das novas tecnologias que vem aparecendo de forma exponencial no mercado estimulando assim mais do que nunca a economia social. O futuro visa uma nova economia que está em transformação, provocando mudanças significativas na política econômica mundial, e por isso, todos os esforços nesta nova dinâmica de conscientização do comportamento social integrativo auxilia numa política estratégica global mais justa e igualitária.

  8. Supernova hydrodynamics experiments using the Nova laser

    Energy Technology Data Exchange (ETDEWEB)

    Remington, B.A.; Glendinning, S.G.; Estabrook, K.; Wallace, R.J.; Rubenchik, A. [Lawrence Livermore National Lab., CA (United States); Kane, J.; Arnett, D. [Arizona Univ., Tucson, AZ (United States). Stewart Observatory; Drake, R.P. [Michigan Univ., Ann Arbor, MI (United States); McCray, R. [Colorado Univ., Boulder, CO (United States)

    1997-04-01

    We are developing experiments using the Nova laser to investigate two areas of physics relevant to core-collapse supernovae (SN): (1) compressible nonlinear hydrodynamic mixing and (2) radiative shock hydrodynamics. In the former, we are examining the differences between the 2D and 3D evolution of the Rayleigh-Taylor instability, an issue critical to the observables emerging from SN in the first year after exploding. In the latter, we are investigating the evolution of a colliding plasma system relevant to the ejecta-stellar wind interactions of the early stages of SN remnant formation. The experiments and astrophysical implications are discussed.

  9. As novas estruturas organizacionais das bolsas

    OpenAIRE

    Marcos Galileu Lorena Dutra

    2008-01-01

    O presente trabalho investiga as novas estruturas organizacionais das bolsas de valores e das bolsas de mercadorias e futuros, implementadas após os processos de desmutualização. É feita uma análise da importância das bolsas para o desenvolvimento econômico, bem como do seu papel de entidades auto-reguladoras. São ainda apresentados os principais fatores que motivaram a conversão das bolsas de associações mutualísticas para sociedades anônimas, bem como as conseqüências dessa alteração organi...

  10. 10% discount at Novae restaurants for students

    CERN Multimedia

    2016-01-01

    A 10% discount will be granted for students dining in restaurants 1 and 2 (on the Meyrin site) during the summer from 15 June 2016 to 15 September 2016.   A special badge will be issued by the respective secretariats if the student fulfils the following criteria:  Is under 25 years old; Is in possession of a student card issued by a University or college; Has a CERN contract > 1 month (Users, Summer Students, Trainees, etc). This badge and the CERN access card will have to be shown at the Novae restaurants in order to benefit from this discount.

  11. As novas estruturas organizacionais das bolsas

    OpenAIRE

    Marcos Galileu Lorena Dutra

    2008-01-01

    O presente trabalho investiga as novas estruturas organizacionais das bolsas de valores e das bolsas de mercadorias e futuros, implementadas após os processos de desmutualização. É feita uma análise da importância das bolsas para o desenvolvimento econômico, bem como do seu papel de entidades auto-reguladoras. São ainda apresentados os principais fatores que motivaram a conversão das bolsas de associações mutualísticas para sociedades anônimas, bem como as conseqüências dessa alteração organi...

  12. Características de carcaça de cordeiros terminados em confinamento, com dietas contendo diferentes níveis protéicos

    Directory of Open Access Journals (Sweden)

    Zundt Marilice

    2003-01-01

    Full Text Available Trinta e dois cordeiros (¹/2 Texel + ¼ Bergamácia + ¼ Corriedale, 16 machos inteiros e 16 fêmeas, foram alimentados durante 71 dias com dietas isoenergéticas (72% NDT, variando os níveis protéicos (12, 16, 20 e 24 % PB em baias individuais, com avaliação de carcaça após abate. O rendimento verdadeiro médio da carcaça foi 54%, enquanto o rendimento comercial médio foi 48%. Verificou-se que os níveis protéicos entre 12 e 24% não afetaram o peso da carcaça quente e fria; o rendimento comercial da carcaça, o índice de compacidade da carcaça e do pernil, bem como a condição corporal, conformação, cobertura de gordura, consistência da gordura, cor da carne, espessura de gordura e deposição de gordura. Os animais terminados com dietas com 12% de proteína bruta foram os que apresentaram maior rendimento verdadeiro de carcaça.

  13. Influência do grupo genético e da alimentação sobre o desempenho de cordeiros em confinamento

    Directory of Open Access Journals (Sweden)

    Barros Nelson Nogueira

    2003-01-01

    Full Text Available O objetivo deste trabalho foi estabelecer a influência do reprodutor e da alimentação sobre o desempenho de cordeiros em confinamento. O delineamento experimental foi o inteiramente casualizado, com arranjo fatorial 2x4, costituído de dois grupos genéticos (Santa Inês x sem raça definida (SRD e Somalis x SRD e concentrado de milho em gão, farelo de soja e sal mineral a 15%, 30%, 45% e 60%. Trinta e dois animais foram confinados em baias individuais e cada um constituiu uma repetição. As dietas eram compostas de feno de leucena (Leucaena leucocephala e concentrado, na forma de ração completa. O aumento de concentrado na dieta dos animais causou incrementos lineares (P0,05 entre os concentrados, porém o grupo genético Somalis x SRD mostrou-se superior (P<0,05 ao Santa Inês x SRD.

  14. Desempenho e características de carcaça de cordeiros alimentados em comedouros privativos recebendo rações contendo semente de girassol Performance and carcass traits of lambs fed diets containing sunflower seed in creep feeding

    Directory of Open Access Journals (Sweden)

    Vicente de Paulo Macedo

    2008-11-01

    Full Text Available Avaliaram-se o desempenho e as características quali e quantitativas da carcaça de cordeiros alimentados com ração contendo semente de girassol. Utilizaram-se 16 cordeiros distribuídos aleatoriamente em um delineamento inteiramente casualizado com quatro tratamentos (0,00; 6,60; 13,20 ou 19,80% de semente de girassol na matéria natural, cada um com quatro repetições, totalizando 16 cordeiros. As dietas continham 2,65; 2,78; 2,89 e 2,93 Mcal/kg de energia metabolizável e 18,38; 18,75; 19,98 e 21,18% de proteína bruta, respectivamente, e foi fornecida ad libitum. Os cordeiros foram pesados a cada 14 dias e mantidos com as ovelhas até atingirem 28 kg, quando foram abatidos, após jejum de sólidos por 18 horas, para obtenção do peso vivo ao abate e registro do peso da carcaça quente e do conteúdo gastrintestinal, utilizados no cálculo do peso de corpo vazio. As carcaças foram mantidas por 24 horas em câmara frigorífica em temperatura de 5ºC para obtenção do peso de carcaça fria. Os níveis de semente de girassol na dieta não afetaram as características de desempenho dos cordeiros. No entanto, os pesos de carcaça quente e de carcaça fria; os pesos de pescoço, baixo, paleta, costela descoberta, costela, lombo; e os rendimentos comerciais de carcaça e costela descoberta, costela, lombo, paleta, pescoço e baixo sofreram efeito da adição da semente de girassol. O fornecimento de semente de girassol na dieta não influencia as características qualitativas e morfométricas da carcaça de cordeiros.Performance and quantitative and qualitative carcass traits of lambs fed with diets containing sunflower seed were evaluated. Sixteen lambs were randomly distributed to a completely randomized design with four diets (0.00, 6.60, 13.20 or 19.80% of sunflower seed, % as fed, with 4 replications. The diets contained 2.65, 2.78, 2.89 and 2.93 Mcal / kg of metabolize energy and 18.38, 18.75, 19.98 and 21.18% crude protein

  15. Efeitos do genótipo e da condição corporal sobre o desempenho de cordeiros terminados em confinamento Effects of genotype group and of the body condition on the performance of lambs finished in feedlot

    Directory of Open Access Journals (Sweden)

    Felipe Queiroga Cartaxo

    2008-08-01

    Full Text Available Avaliaram-se o desempenho e a margem bruta de lucro de cordeiros terminados em confinamento. Foram utilizados 32 cordeiros não-castrados - 16 Santa Inês (SI e 16 ½ Dorper × ½ Santa Inês (DpSI - com 103 dias de idade e 20,0 kg de peso corporal. Os cordeiros receberam ração completa com 30% de feno de maniçoba (Manihot pseudoglaziovii e 70% de concentrado. O período de adaptação às instalações e à dieta foi de 14 dias. O delineamento experimental foi inteiramente casualizado em esquema fatorial 2 × 2, composto de dois genótipos e dois escores corporais. Não foi observado efeito significativo dos genótipos sobre nenhuma característica de desempenho estudada, contudo, os mestiços (DpSI possibilitaram maior margem bruta de lucro. A condição corporal afetou significativamente o consumo de matéria seca, a conversão alimentar e o número de dias em confinamento. Os cordeiros com condição corporal intermediária consumiram 1,04 kg/dia e 82,64 g/kg0,75, enquanto aqueles com condição gorda consumiram 1,15 kg/dia e 86,79 g/kg0,75. Os cordeiros com condição corporal intermediária apresentaram menor consumo de matéria seca e melhor conversão alimentar, o que resultou em menor número de dias em confinamento e maior margem bruta de lucro em comparação aos cordeiros com condição corporal gorda, independentemente do genótipo.The objective of this study was to evaluate the performance and the gross margin of profit of lambs finished in feedlot. Thirty-two no castrate male lambs from the genotype Santa Inês and crossbred Dorper × Santa Inês and two body condition, intermediate and fat, were used. The lambs were 16 Santa Inês (SI and 16 ½ Dorper × ½ Santa Inês (DpSI, with average 103 days old and 20.0 kg BW. The lambs were full fed ration with 30% of maniçoba hay (Manihot pseudoglaziovii and 70% of concentrate. The adaptation period to the installation and the diet was of 14 days. A completely randomized design in a

  16. The Nova Rate in M94 (NGC4736)

    CERN Document Server

    Gueth, T; Misselt, K A

    2010-01-01

    A multi-epoch H$\\alpha$ survey of the early-type spiral galaxy M94 (NGC 4736) has been completed as part of a program to establish the galaxy's nova rate. A total of 4 nova candidates were discovered in 7 epochs of observation during the period from 2005 to 2007. After making corrections for temporal coverage and spatial completeness, a global nova rate of 5.0$^{+1.8}_{-1.4}$ yr$^{-1}$ was determined. This rate corresponds to a specific-luminosity nova rate of 1.4 $\\pm$ 0.5 novae per year per 10$^{10} L_{\\odot,K}$ when the K luminosity is determined from the B - K color, or 1.5 $\\pm$ 0.4 novae per year per 10$^{10} L_{\\odot,K}$ when the K luminosity is derived from the Two Micron All Sky Survey. These values are slightly lower than that of other galaxies with measured nova rates, which typically lie in the range of 2-3 novae per year per 10$^{10} L_{\\odot}$ in the K band.

  17. A Spectroscopic and Photometric Survey of Novae in M31

    CERN Document Server

    Shafter, A W; Hornoch, K; Filippenko, A V; Bode, M F; Ciardullo, R; Misselt, K A; Hounsell, R A; Chornock, R; Matheson, T

    2011-01-01

    We report the results of a multi-year spectroscopic and photometric survey of novae in M31 that resulted in a total of 53 spectra of 48 individual nova candidates. Two of these, M31N 1995-11e and M31N 2007-11g, were revealed to be long-period Mira variables, not novae. These data double the number of spectra extant for novae in M31 through the end of 2009 and bring to 91 the number of M31 novae with known spectroscopic classifications. We find that 75 novae (82%) are confirmed or likely members of the Fe II spectroscopic class, with the remaining 16 novae (18%) belonging to the He/N (and related) classes. These numbers are consistent with those found for Galactic novae. We find no compelling evidence that spectroscopic class depends sensitively on spatial position or population within M31 (i.e., bulge vs. disk), although the distribution for He/N systems appears slightly more extended than that for the Fe II class. We confirm the existence of a correlation between speed class and ejection velocity (based on l...

  18. The progenitor of Nova Cygni 2006 (=V2362 Cyg)

    NARCIS (Netherlands)

    Steeghs, D.; Greimel, R.; Drew, J.; Irwin, M.; Gaensicke, B.; Groot, P.J.; Knigge, C.

    2006-01-01

    We report on the detection of the likely progenitor to Nova Cygni 2006 = V2362 Cyg (IAUC #8697, #8698, ATel #792) using images from the INT Photometric H-Alpha Survey (IPHAS; http://www.iphas.org). The field containing the classical nova was observed as part of our galactic plane survey on Aug. 3rd

  19. Some misapplied nomina nova in reef coral taxonomy (Scleractinia)

    NARCIS (Netherlands)

    Hoeksema, B.W.

    1993-01-01

    Nomina nova should be used only to denote replacement names for preoccupied names, i.e. in the case of homonymy. Three examples of incorrect applications of nomina nova in scleractinian taxonomy are given. Coincidentally, in the cases discussed each wrongly proposed nomen novum concerns a new specie

  20. Results of Statewide TerraNova Testing, Fall 1998.

    Science.gov (United States)

    La Marca, Paul M.

    This summary provides key findings about state, district, and school level performance on the TerraNova examinations (CTB/McGraw Hill) in Nevada in 1998-1999. The TerraNova tests are used to assess students in grades 4, 8, and 10 as stipulated by Nevada law. Within this summary, a description of performance as measured by national percentile…

  1. NOVA: a software to analyze complexome profiling data

    NARCIS (Netherlands)

    Giese, H.; Ackermann, J.; Heide, H.; Bleier, L.; Drose, S.; Wittig, I.; Brandt, U.; Koch, I.

    2015-01-01

    SUMMARY: We introduce nova, a software for the analysis of complexome profiling data. nova supports the investigation of the composition of complexes, cluster analysis of the experimental data, visual inspection and comparison of experiments and many other features. AVAILABILITY AND IMPLEMENTATION:

  2. Época de nascimento sobre a composição regional e tecidual da carcaça de cordeiros da raça Texel Birth season on regional and tissue carcass composition in Texel breed lambs

    Directory of Open Access Journals (Sweden)

    Gilson de Mendonça

    2008-06-01

    Full Text Available Foram avaliados os efeitos de épocas alternativas de nascimento sobre a composição regional e tecidual da carcaça em ovinos. Quarenta e nove cordeiros machos não-castrados da raça Texel, nascidos em duas épocas (agosto e novembro, foram mantidos em regime de pastagem e abatidos com média de idade de 129 e 164 dias, respectivamente. Previamente aos abates foi feita a avaliação da produção forrageira do campo pelo método Botanal. Foram verificadas melhores condições forrageiras para os cordeiros nascidos em agosto, que apresentaram maior peso e proporção na maioria dos cortes, assim como menor proporção de músculo na paleta e perna; apresentando maior conteúdo de tecido adiposo na maioria dos cortes da carcaça. Para os cordeiros nascidos em novembro, ocorreu maior relação músculo:gordura e músculo:osso na paleta e na perna, assim como maior relação músculo:gordura no costilhar. As condições nutricionais são responsáveis pelas diferenças nos pesos e rendimentos dos cortes, assim como na composição tecidual da carcaça, em cordeiros mantidos em regime de pasto, viabilizando o uso de época alternativa de nascimentos para incrementar a oferta de animais para o abate.The effect of alternative birth season on regional and tissue carcass composition of sheep was evaluated. Forty nine (49 Texel intact male lambs, born in two seasons (August and November, were kept under grazing and slaughtered with an average age of 129 and 164 days, respectively. Prior to slaughter forage production was measured using Botanal method. Lambs born in August had more favorable forage conditions, showing higher body weight and proportion in the majority of cuts, as well as lower proportion of shoulder and leg muscles showing higher adipose tissue content in the majority of carcass cuts. For lambs born in November, a higher muscle:fat and muscle:bone rate in shoulder and leg, as well as a higher ribcut muscle:fat rate. Nutritional

  3. Desempenho, consumo e morfometria in vivo de cordeiros Santa Inês alimentados com rações contendo torta de girassol em substituição ao farelo de algodão

    Directory of Open Access Journals (Sweden)

    F. Fernandes Júnior

    2015-04-01

    Full Text Available Este estudo foi conduzido com o objetivo de determinar o melhor teor de substituição da proteína do farelo de algodão pela proteína da torta de girassol em dietas para cordeiros Santa Inês, por meio da avaliação do consumo, ganho de peso, conversão alimentar e medidas morfométricas. Foram confinados, por 60 dias, 30 cordeiros da raça Santa Inês, machos inteiros, com idade e peso médio no início do experimento de 80 dias e 21,45±2,16kg, respectivamente. O delineamento experimental foi completamente casualizado, sendo os animais divididos em 5 tratamentos, com 6 repetições por tratamento, de acordo com a quantidade de proteína do farelo de algodão substituída pela proteína da torta de girassol (0, 20, 40, 60 e 80% de substituição. As variáveis peso final, consumo de matéria seca e conversão alimentar não foram afetadas pelas dietas experimentais, embora o ganho médio diário tenha sido inferior para as dietas com maior teor de torta de girassol. Para os parâmetros de consumo, verificou-se diferença apenas no consumo de extrato etéreo em relação ao peso metabólico (g/kg PV0,75, em que cordeiros recebendo dieta com maior teor de torta de girassol ingeriram maiores quantidades de extrato etéreo. Em relação às medidas morfométricas, houve decréscimo linear da altura de dorso e largura de garupa com a inclusão da torta de girassol na dieta. A substituição da proteína do farelo de algodão pela proteína da torta de girassol afetou negativamente o ganho de peso de cordeiros Santa Inês em confinamento. Porém, teve pouca ou nenhuma influência nos parâmetros de consumo e nas medidas morfométricas in vivo.

  4. Legislating Interprofessional Regulatory Collaboration in Nova Scotia

    Directory of Open Access Journals (Sweden)

    William Lahey

    2013-10-01

    Full Text Available To shift health professions regulation from traditional to ‘collaborative’ self-regulation, Nova Scotia has adopted legislation which will: make all self-regulating health professions members of the Regulated Health Professions Network; mandate the Network to facilitate voluntary collaboration among its members; and enable regulators to work together on investigations of patient complaints, to adjust scopes of practice on an ongoing basis and to adjudicate appeals of unsuccessful applicants for registration. The goals are to give health professions regulation the capacity to enable and support the functioning of interprofessional teams. The legislation was adopted primarily for two reasons: collaborative development and unanimous support by all of the province’s self-regulating professions; and alignment with the government’s health care reform agenda and its emphasis on collaborative team-based care. Contrary to the approach of several other provinces, the legislation will enable but not require regulators to collaborate on the premise that consensual collaboration is more likely to happen, to be meaningful and to yield tangible benefits. Support for this approach can be taken from the impressive collaborative work on which the legislation is based. Evaluation will be critical, and the five-year review required by the legislation will give Nova Scotia the opportunity to test not only the legislation but the ideas on which it is based. The extent of the legislation’s reliance on voluntary process will prove to be either its greatest strength or its greatest weakness.

  5. Characterization of Dwarf Novae Using SDSS Colors

    CERN Document Server

    Kato, Taichi; Uemura, Makoto

    2011-01-01

    We have developed a method for estimating orbital periods of dwarf novae from SDSS colors in quiescence using an artificial neural network. For typical objects below the period gap with good photometric accuracy, we could estimate orbital periods to a 1-sigma error of 22%. The error of estimation is worse for systems with longer periods. We have also developed a neural network-based method for categorical classification. This method has been proven to be efficient in classifying objects into three categories (WZ Sge-type, SU UMa-type and SS Cyg/Z Cam-type) and works for very faint objects down to g=21. Using these methods, we have investigated the distribution of orbital periods of dwarf novae from a modern transient survey (Catalina Real-Time Survey). Using Bayesian analysis developed by Uemura et al. (2010, arXiv:1003.0945), the present sample tends to give a flatter distribution toward the shortest period and a shorter estimate of the period minimum, which may have been resulted from the uncertainties in t...

  6. The nature and evolution of Nova Cygni 2006

    CERN Document Server

    Munari, U; Henden, A; Cardarelli, G; Cherini, G; Dallaporta, S; Via, G Dalla; Frigo, A; Jurdana-Sepic, R; Moretti, S; Ochner, P; Tomaselli, S; Tomasoni, S; Valisa, P; Navasardyan, H; Valentini, M

    2008-01-01

    AIMS: Nova Cyg 2006 has been intensively observed throughout its full outburst. We investigate the energetics and evolution of the central source and of the expanding ejecta, their chemical abundances and ionization structure, and the formation of dust. METHOD: We recorded low, medium, and/or high-resolution spectra (calibrated into accurate absolute fluxes) on 39 nights, along with 2353 photometric UBVRcIc measures on 313 nights, and complemented them with IR data from the literature. RESULTS: The nova displayed initially the normal photometric and spectroscopic evolution of a fast nova of the FeII-type. Pre-maximum, principal, diffuse-enhanced, and Orion absorption systems developed in a normal way. After the initial outburst, the nova progressively slowed its fading pace until the decline reversed and a second maximum was reached (eight months later), accompanied by large spectroscopic changes. Following the rapid decline from second maximum, the nova finally entered the nebular phase and formed optically ...

  7. Observations and simulations of nova Vul 1984 no. 2: A nova with ejecta rich in oxygen, neon, and magnesium

    Science.gov (United States)

    Starrfield, S.; Sonneborn, G.; Stryker, L. L.; Sparks, Warren M.; Truran, James W.; Ferland, Gary; Wagner, R. M.; Gallagher, J. S.; Wade, R.; Williams, R. E.

    1988-01-01

    Nova Vul 1984 no. 2 was observed with IUE from Dec. 1984 through Nov. 1987. The spectra are characterized by strong lines from Mg, Ne, C, Si, O, N, and other elements. Data obtained in the ultraviolet, infrared, and optical show that this nova is ejecting material rich in oxygen, neon, and magnesium.

  8. 20 December 2013 - R. M. Cordeiro Dunlop Ambassador Permanent Representative of Brazil to the United Nations Office and other international organisations in Geneva visiting the LHC tunnel at Point 5 with CMS Collaboration, CERN Team Leader A. Petrilli and signing the Guest Book with CERN Director-General. Accompanied by J. Salicio and R. Voss throughout.

    CERN Document Server

    Jean-Claude Gadmer

    2013-01-01

    20 December 2013 - R. M. Cordeiro Dunlop Ambassador Permanent Representative of Brazil to the United Nations Office and other international organisations in Geneva visiting the LHC tunnel at Point 5 with CMS Collaboration, CERN Team Leader A. Petrilli and signing the Guest Book with CERN Director-General. Accompanied by J. Salicio and R. Voss throughout.

  9. The panchromatic spectroscopic evolution of the classical CO nova V339 Del (Nova Del 2013) until X-ray turnoff

    CERN Document Server

    Shore, S N; Schwarz, G J; Teyssier, F M; Buil, C; Aquino, I De Gennaro; Page, K L; Osborne, J P; Scaringi, S; Starrfield, S; van Winckel, H; Williams, R E; Woodward, C E

    2016-01-01

    Classical novae are the product of thermonuclear runaway-initiated explosions occurring on accreting white dwarfs. V339 Del (Nova Delphinus 2013) was one of the brightest classical novae of the last hundred years. Spectroscopy and photometry are available from $\\gamma$-rays through infrared at stages that have frequently not been well observed. The complete data set is intended to provide a benchmark for comparison with modeling and for understanding more sparsely monitored historical classical and recurrent novae. This paper is the first in the series of reports on the development of the nova. We report here on the early stages of the outburst, through the X-ray active stage. A time sequence of optical, flux calibrated high resolution spectra was obtained with the Nordic Optical Telescope (NOT) using FIES simultaneously, or contemporaneously, with the Space Telescope Imaging Spectrograph (STIS) aboard the Hubble Space Telescope during the early stages of the outburst. These were supplemented with MERCATOR/HE...

  10. Nova Scotia Power response to Hurricane Juan

    Energy Technology Data Exchange (ETDEWEB)

    NONE

    2003-10-01

    Hurricane Juan hit the Halifax Regional Municipality on September 28, 2003, creating the largest outage in Nova Scotia Power's history. This detailed report documents the extensive damage that Hurricane Juan caused to the power transmission and distribution system in Nova Scotia. It also reviews the massive power restoration effort, with reference to numerous interviews, computer records and data logs which offer a wide range of observations, statistics and insights into the preparation and performance of Nova Scotia Power Inc. (NSPI) and the efforts of other key organizations following the storm. NSPI organized a recovery effort that matched the intensity of the hurricane. A fire in the Scotia Square Office Tower caused the evacuation of the company's call centre. The Tufts Cove station in Dartmouth, which generates 400 megawatts of power, was forced to shut down. Excess electricity was moved into New Brunswick and other jurisdictions to maintain system stability. The main priority was to restore customers back to service. Within 5 days of the hurricane, 95 per cent of those who lost power had service restored. Hurricane Juan caused the most damage to the transmission and distribution system in NSPI's history. Three out of five high capacity transmission lines were put out of service. Three 120-foot high transmission towers fell, and 17 main transmission lines were damaged and put out of service. Forty-five major substations were affected and 145 distribution feeders were damaged or tripped off, including 106 in the Halifax Regional Municipality. Large portions of 4,500 kilometres of local distribution lines in the Halifax Regional Municipality were damaged, including thousands of kilometers across the Northeast. The power crew, consisting of 2,000 individuals from the region and neighbouring utilities in New Brunswick and Maine, worked for 15 consecutive days to replace 275 transformers, 760 power poles, and 125,000 metres of conductor wire. NSPI

  11. Ciberespaço: nova realidade, novos perigos, novas formas de defesa

    Directory of Open Access Journals (Sweden)

    Ana Maria Nicolaci-da-Costa

    Full Text Available A mídia, nacional e internacional, vem divulgando à exaustão vários tipos de perigo que supostamente rondam a utilização da Internet. Por trás dessa divulgação, parece estar um pressuposto que desafia a Psicologia: o de que somos indefesos para lidar com a nova realidade do ciberespaço. Resultados inesperados de uma pesquisa sobre o uso intensivo da Internet, no entanto, mostram o contrário. A partir destes, novas estratégias de auto-proteção online, que visam principalmente à preservação da intimidade, puderam ser identificadas. Essas estratégias envolvem diferentes formas de utilização, por parte dos usuários, dos próprios programas e recursos tecnológicos disponíveis.

  12. Laying the foundation for a digital Nova Scotia

    Science.gov (United States)

    Bond, J.

    2016-04-01

    In 2013, the Province of Nova Scotia began an effort to modernize its coordinate referencing infrastructure known as the Nova Scotia Coordinate Referencing System (NSCRS). At that time, 8, active GPS stations were installed in southwest Nova Scotia to evaluate the technology's ability to address the Province's coordinate referencing needs. The success of the test phase helped build a business case to implement the technology across the entire Province. It is anticipated that by the end of 2015, 40 active GPS stations will be in place across Nova Scotia. This infrastructure, known as the Nova Scotia Active Control Stations (NSACS) network, will allow for instantaneous, centimetre level positioning across the Province. Originally designed to address the needs of the surveying community, the technology has also proven to have applications in mapping, machine automation, agriculture, navigation, emergency response, earthquake detection and other areas. In the foreseeable future, all spatial data sets captured in Nova Scotia will be either directly or indirectly derived from the NSACS network. The technology will promote high accuracy and homogenous spatial data sets across the Province. The technology behind the NSACS and the development of the system are described. Examples of how the technology is contributing to a digital Nova Scotia are presented. Future applications of the technology are also considered.

  13. OGLE Atlas of Classical Novae II. Magellanic Clouds

    CERN Document Server

    Mroz, P; Poleski, R; Soszynski, I; Szymanski, M K; Pietrzynski, G; Wyrzykowski, L; Ulaczyk, K; Kozlowski, S; Pietrukowicz, P; Skowron, J

    2016-01-01

    The population of classical novae in the Magellanic Clouds was poorly known because of a lack of systematic studies. There were some suggestions that nova rates per unit mass in the Magellanic Clouds were higher than in any other galaxy. Here, we present an analysis of data collected over sixteen years by the OGLE survey with the aim of characterizing nova population in the Clouds. We found twenty eruptions of novae, half of them are new discoveries. We robustly measure the nova rates of $2.4 \\pm 0.8$ yr$^{-1}$ (LMC) and $0.9 \\pm 0.4$ yr$^{-1}$ (SMC) and confirm that K-band luminosity-specific nova rates in both Clouds are 2-3 times higher than in other galaxies. This can be explained by the star formation history in the Magellanic Clouds, specifically a re-ignition of the star formation rate a few Gyr ago. We also present the discovery of an intriguing system OGLE-MBR133.25.1160 which mimics recurrent nova eruptions.

  14. OGLE Atlas of Classical Novae. II. Magellanic Clouds

    Science.gov (United States)

    Mróz, P.; Udalski, A.; Poleski, R.; Soszyński, I.; Szymański, M. K.; Pietrzyński, G.; Wyrzykowski, Ł.; Ulaczyk, K.; Kozłowski, S.; Pietrukowicz, P.; Skowron, J.

    2016-01-01

    The population of classical novae in the Magellanic Clouds was poorly known because of a lack of systematic studies. There were some suggestions that nova rates per unit mass in the Magellanic Clouds were higher than in any other galaxy. Here, we present an analysis of data collected over 16 years by the OGLE survey with the aim of characterizing the nova population in the Clouds. We found 20 eruptions of novae, half of which are new discoveries. We robustly measure nova rates of 2.4 ± 0.8 yr-1 (LMC) and 0.9 ± 0.4 yr-1 (SMC) and confirm that the K-band luminosity-specific nova rates in both Clouds are 2-3 times higher than in other galaxies. This can be explained by the star formation history in the Magellanic Clouds, specifically the re-ignition of the star formation rate a few Gyr ago. We also present the discovery of the intriguing system OGLE-MBR133.25.1160, which mimics recurrent nova eruptions.

  15. The Unusually Luminous Extragalactic Nova SN 2010U

    CERN Document Server

    Czekala, Ian; Chornock, R; Pastorello, A; Marion, G H; Margutti, R; Botticella, M T; Challis, P; Ergon, M; Smartt, S; Sollerman, J; Vinkó, J; Wheeler, J C

    2012-01-01

    We present observations of the unusual optical transient SN 2010U, including spectra taken 1.03 days to 15.3 days after maximum light that identify it as a fast and luminous Fe II type nova. Our multi-band light curve traces the fast decline (t_2 = 3.5 days) from maximum light (M_V = -10.2 mag), placing SN 2010U in the top 0.5% of the most luminous novae ever observed. We find typical ejecta velocities of approximately 1100 km/s and that SN 2010U shares many spectral and photometric characteristics with two other fast and luminous Fe II type novae, including Nova LMC 1991 and M31N-2007-11d. For the extreme luminosity of this nova, the maximum magnitude vs. rate of decline relationship indicates a massive white dwarf progenitor with a low pre-outburst accretion rate. However, this prediction is in conflict with emerging theories of nova populations, which predict that luminous novae from massive white dwarfs should preferentially exhibit an alternate spectral type (He/N) near maximum light.

  16. CLIP Identifies Nova-Regulated RNA Networks in the Brain

    Science.gov (United States)

    Ule, Jernej; Jensen, Kirk B.; Ruggiu, Matteo; Mele, Aldo; Ule, Aljaž; Darnell, Robert B.

    2003-11-01

    Nova proteins are neuron-specific antigens targeted in paraneoplastic opsoclonus myoclonus ataxia (POMA), an autoimmune neurologic disease characterized by abnormal motor inhibition. Nova proteins regulate neuronal pre-messenger RNA splicing by directly binding to RNA. To identify Nova RNA targets, we developed a method to purify protein-RNA complexes from mouse brain with the use of ultraviolet cross-linking and immunoprecipitation (CLIP). Thirty-four transcripts were identified multiple times by Nova CLIP. Three-quarters of these encode proteins that function at the neuronal synapse, and one-third are involved in neuronal inhibition. Splicing targets confirmed in Nova-/- mice include c-Jun N-terminal kinase 2, neogenin, and gephyrin; the latter encodes a protein that clusters inhibitory γ-aminobutyric acid and glycine receptors, two previously identified Nova splicing targets. Thus, CLIP reveals that Nova coordinately regulates a biologically coherent set of RNAs encoding multiple components of the inhibitory synapse, an observation that may relate to the cause of abnormal motor inhibition in POMA.

  17. MESA and NuGrid Simulations of Classical Nova Outbursts: ONe Nova and Nucleosynthesis

    CERN Document Server

    Denissenkov, Pavel A; Pignatari, Marco; Trappitsch, Reto; Ritter, Christian; Herwig, Falk; Battino, Umberto; Setoodehnia, Kiana

    2013-01-01

    Classical novae are the result of thermonuclear flashes of H accreted by CO or ONe white dwarfs, leading eventually to the dynamic ejection of the surface layers. These are observationally known to be enriched in heavy elements, such as C, O and Ne that must originate in layers below the H-flash convection zone. Building on our previous work we now present stellar evolution simulations of ONe nova, and provide a comprehensive comparison of our models with previous work. Some of our models include exponential convective boundary mixing model to account for the observed enrichment of the ejecta even when accreting material with a solar abundance distribution. Our models produce maximum temperature evolution profiles and nucleosynthesis yields in good agreement with models that generate enriched ejecta by assuming that the accreted material was pre-enriched. We confirm for ONe nova the result we reported previously, i.e. we found that 3He can be produced in situ in solar-composition envelopes accreted with slow ...

  18. Nova abordagem no tratamento da esquizofrenia

    Directory of Open Access Journals (Sweden)

    Walter Speltri

    1966-12-01

    Full Text Available Foram tratados 11 casos de esquizofrenia com a guanetidina, substância considerada, do ponto de vista farmacodinâmico, como simpaticoplégica. Na opinião do autor, os surpreendentes e significativos resultados obtidos autorizam uma nova abordagem nas pesquisas à procura da etiopatogenia da esquizofrenia e, a partir dos elementos colhidos, considera plausível uma "teoria psicossomática da esquizofrenia". Recusa-se, entretanto, a cair no atraente, mas inútil, terreno especulativo. Prefere aguardar que os farmacologistas e fisiologistas forneçam dados pais precisos sobre o mecanismo de ação da guanetidina e que novos estudos confirmem seus resultados para, depois, dar publicidade à sua teoria.

  19. Novas tecnologias: Novos Professores? Novos Saberes?

    Directory of Open Access Journals (Sweden)

    Daniele Cristina Mendes

    2008-11-01

    Full Text Available RESUMO:A integração da educação com a informação-comunicação precisa ter seu lugar repensado dentro das escolas. Neste artigo tento instigar reflexões no trato das questões referentes às novas tecnologias e suas implicações na leitura, na linguagem e na formação dos professores.PALAVRAS-CHAVE: Leitura, Internet, Formação DocenteABSTRACT:The integration of education with the information and communication, must have rethought its place within the schools. In this article I try to instigate reflections on issues concerning the treatment of new technologies and their implications for reading, in language and training of teachers.KEYWORDS: Reading, Internet, Teacher educationRecebido: 30/10/2008     Aceito:30/11/2008

  20. La nova identitat visual de la EAP

    Directory of Open Access Journals (Sweden)

    Dario D. Aguillón Gutiérrez

    2015-01-01

    Full Text Available L'Escola d'Arts Plàstiques de la Universitat Autònoma de Coahuila, a Mèxic, ha estat durant dècades una de les institucions d'ensenyament d'art i disseny més importants al nord del país. Les seves necessitats de comunicació actuals, així com la seva constant creixement, van fer necessari el disseny d'una nova identitat visual, coherent amb la seva personalitat i conscient de l'entorn en què es desenvolupa. Aquest projecte va ser realitzat entre directius, docents i estudiants de l'Escola d'Arts Plàstiques, amb l'objectiu de dotar la institució d'una identitat pròpia i professional.

  1. Newly Identified Rydberg Emission Lines in Novae

    Science.gov (United States)

    Lynch, David K.; Rudy, R. J.; Bernstein, L. S.

    2008-09-01

    Newly Identified Rydberg Emission Lines in Novae David K. Lynch, Richard. J. Rudy (The Aerospace Corporation) & Lawrence S. Bernstein (Spectral Sciences, Inc.) Novae spectra in the near infrared frequently show a set of six emission lines that have not been positively identified (Williams, Longmore, & Geballe 1996, MNRAS, 279, 804; Lynch et al. 2001, AJ, 122, 2013; Rudy et al. 2002 ApJ, 573, 794; Lynch et al. 2004 Astron. J. 127, 1089-1097). These lines are at 0.8926, 1.1114, 1.1901, 1.5545, 2.0996 and 2.425 µm ± 0.005 µm. Krautter et al. (1984 A&A 137, 304) suggested that three of the lines were due to rydberg (hydrogenic) transitions in an unspecified atomic species that was in the 4th or 5th ionization stage (core charge = 4 & 5). We believe that Krautter et al.'s explanation is correct based on 4 additional lines that we have identified in the visible and near infrared spectrum of V723 Cassiopeiae. The observed Rydberg lines appear to originate from high angular momentum states with negligible quantum defects. The species cannot be determined with any certainty because in rydberg states, the outer electron sees a nucleus shielded by the inner electrons and together the inner atom appears to have a charge of +1, like hydrogen. As a result, the atom looks hydrogenic and species such as CV, NV, OV, MgV, SiV, etc. have their rydberg transitions at very similar wavelengths. All the lines represent permitted transitions, most likely formed by recombination. Atoms with core charges 4, 5 & 6 are rarely seen in the astrophysical environment because an extremely hot radiation field is necessary to ionize them. Thermonuclear runaways on the surface of a white dwarf can reach millions of degrees K, and thus there are enough X-ray photons available to achieve the necessary high ionization levels.

  2. Light Curve Analysis of Neon Novae

    CERN Document Server

    Hachisu, Izumi

    2015-01-01

    We analyzed light curves of five neon novae, QU Vul, V351 Pup, V382 Vel, V693 CrA, and V1974 Cyg, and determined their white dwarf (WD) masses and distance moduli on the basis of theoretical light curves composed of free-free and photospheric emission. For QU Vul, we obtained a distance of d~2.4 kpc, reddening of E(B-V)~0.55, and WD mass of M_WD=0.82-0.96 M_sun. This suggests that an oxygen-neon WD lost a mass of more than ~0.1 M_sun since its birth. For V351 Pup, we obtained d~5.5 kpc, E(B-V)~0.45, and M_WD=0.98-1.1 M_sun. For V382 Vel, we obtained d~1.6 kpc, E(B-V)~0.15, and M_WD=1.13-1.28 M_sun. For V693 CrA, we obtained d~7.1 kpc, E(B-V)~0.05, and M_WD=1.15-1.25 M_sun. For V1974 Cyg, we obtained d~1.8 kpc, E(B-V)~0.30, and M_WD=0.95-1.1 M_sun. For comparison, we added the carbon-oxygen nova V1668 Cyg to our analysis and obtained d~5.4 kpc, E(B-V)~0.30, and M_WD=0.98-1.1 M_sun. In QU Vul, photospheric emission contributes 0.4-0.8 mag at most to the optical light curve compared with free-free emission only....

  3. Estação de nascimento e puberdade em cordeiros Santa Inês Season of birth and puberty in Santa Inês lambs

    Directory of Open Access Journals (Sweden)

    Jordan Meneses Alves

    2006-06-01

    Full Text Available Neste estudo, investigou-se o efeito da estação de nascimento sobre a puberdade de cordeiros Santa Inês criados no Distrito Federal. Utilizaram-se 33 cordeiros machos, inteiros, distribuídos em quatro lotes de grupos contemporâneos. A diferença de idade de cada grupo foi de 90 dias, abrangendo as quatro estações do ano. Foram realizadas coletas de dados mensalmente e a cada 15 dias, dependendo da presença ou ausência de espermatozóides no ejaculado de cada animal. A puberdade foi definida quando o sêmen do animal apresentou motilidade total de 10% e concentração espermática de 50 x 10(6 espermatozóides por mililitro (mL de ejaculado. Após a definição da puberdade, procedeu-se a mais uma coleta e, após 15 dias, realizou-se a castração dos animais. A idade à puberdade dos animais foi de 194,57 ± 41,97 dias. A estação do ano afetou a idade à puberdade entre os grupos, principalmente em razão do fator nutricional, visto que os pesos à puberdade foram semelhantes. O grupo mais precoce (nascido em agosto apresentou idade à puberdade de 162,56 ± 35,55 dias. Correlações significativas foram encontradas entre peso e circunferência escrotal (CE, comprimento e largura testicular, sugerindo que a CE pode ser utilizada como critério complementar para a seleção feita com base nos parâmetros produtivos.The present study investigated the effect of calving season on puberty of Santa Inês ram lambs raised in the Distrito Federal, Brazil. Thirty-three ram lambs were assigned to four contemporary groups according to birth date, distributed in three months intervals. Data were collected monthly and every 15 days depending on the presence of sperm in each animal ejaculate. Puberty was defined when the animal presented total motility of 10% and sperm concentration of 50 x 10(6 per mL of ejaculated semen. This procedure was repeated after puberty and after 15 days the animals were castrated. Mean age at puberty was 194.57 ± 41

  4. Ultraviolet spectroscopy of old novae and symbiotic stars

    Science.gov (United States)

    Lambert, D. L.; Slovak, M. H.; Shields, G. A.; Ferland, G. J.

    1981-01-01

    The IUE spectra are presented for two old novae and for two of the symbiotic variables. Prominent emission line spectra are revealed as a continuum whose appearance is effected by the system inclination. These data provide evidence for hot companions in the symbiotic stars, making plausible the binary model for these peculiar stars. Recent IUE spectra of dwarf novae provide additional support for the existence of optically thick accretion disks in active binary systems. The ultraviolet data of the eclipsing dwarf novae EX Hya and BV Cen appear flatter than for the noneclipsing systems, an effect which could be ascribed to the system inclination.

  5. Distributed computer control system in the Nova Laser Fusion Test Facility

    Energy Technology Data Exchange (ETDEWEB)

    1985-09-01

    The EE Technical Review has two purposes - to inform readers of various activities within the Electronics Engineering Department and to promote the exchange of ideas. The articles, by design, are brief summaries of EE work. The articles included in this report are as follows: Overview - Nova Control System; Centralized Computer-Based Controls for the Nova Laser Facility; Nova Pulse-Power Control System; Nova Laser Alignment Control System; Nova Beam Diagnostic System; Nova Target-Diagnostics Control System; and Nova Shot Scheduler. The 7 papers are individually abstracted.

  6. Very high energy gamma-ray follow-up observations of novae and dwarf novae with the MAGIC telescopes

    CERN Document Server

    López-Coto, R; Bednarek, W; Desiante, R; Longo, F

    2015-01-01

    In the last few years the Fermi-LAT instrument has detected GeV gamma-ray emission from several novae. Such GeV emission can be interpreted in terms of inverse Compton emission from electrons accelerated in the shock or in terms of emission from hadrons accelerated in the same conditions. The latter might reach much higher energies and could produce a second component in the gamma-ray spectrum at TeV energies. We perform follow-up observations of selected novae and dwarf novae in search of the second component in TeV energy gamma rays. This can shed light on the acceleration process of leptons and hadrons in nova explosions. We have performed observations with the MAGIC telescopes of 3 sources, a symbiotic nova YY Her, a dwarf nova ASASSN-13ax and a classical nova V339 Del, shortly after their outbursts. We did not detect TeV gamma-ray emission from any of the objects observed. The TeV upper limits from MAGIC observations and the GeV detection by Fermi constrain the acceleration parameters for electrons and h...

  7. The spectroscopic evolution of the $\\gamma$-ray emitting classical nova Nova Mon 2012. I. Implications for the ONe subclass of classical novae

    CERN Document Server

    Shore, S N; Schwarz, G J; Augusteijn, T; Cheung, C C; Walter, F M; Starrfield, S

    2013-01-01

    Nova Mon 2012 was the first classical nova to be detected as a high energy $\\gamma$-ray transient, by Fermi-LAT, before its optical discovery. We study a time sequence of high resolution optical echelle spectra (Nordic Optical Telescope) and contemporaneous NOT, STIS UV, and CHIRON echelle spectra (Nov 20/21/22). We use [O III] and H$\\beta$ line fluxs to constrain the properties of the ejecta. We derive the structure from the optical and UV line profiles and compare our measured line fluxes for with predictions using Cloudy with abundances from other ONe novae. Mon 2012 is confirmed as an ONe nova. We find E(B-V)=0.85$\\pm$0.05 and hydrogen column density $\\approx 5\\times 10^{21}$ cm$^{-2}$. The corrected continuum luminosity is nearly the same in the entire observed energy range as V1974 Cyg, V382 Mon, and Nova LMC 2000 at the same epoch after outburst. The distance, about 3.6 kpc, is quite similar to V1974 Cyg. The line profiles can be modeled using an axisymmetric bipolar geometry for the ejecta with variou...

  8. Ocean and Coastal Acidification off New England and Nova Scotia

    Science.gov (United States)

    New England coastal and adjacent Nova Scotia shelf waters have a reduced buffering capacity because of significant freshwater input, making the region’s waters potentially more vulnerable to coastal acidification. Nutrient loading and heavy precipitation events further acid...

  9. Gamma-ray emission from individual classical novae

    CERN Document Server

    Gómez-Gomar, J; José, J; Isern, J

    1997-01-01

    Classical novae are important producers of radioactive nuclei, such as be7, n13, f18, na22 and al26. The disintegration of these nuclei produces positrons (except for be7) that through annihilation with electrons produce photons of energies 511 keV and below. Furthermore, be7 and na22 decay producing photons with energies of 478 keV and 1275 keV, respectively, well in the gamma-ray domain. Therefore, novae are potential sources of gamma-ray emission. The properties of gamma-ray spectra and gamma-ray light curves (for the continuum and for the lines at 511, 478 and 1275 keV) have been analyzed, with a special emphasis on the difference between carbon-oxygen and oxygen-neon novae. Predictions of detectability of individual novae by the future SPI spectrometer on board the INTEGRAL satellite are made.

  10. Ocean and Coastal Acidification off New England and Nova Scotia

    Science.gov (United States)

    New England coastal and adjacent Nova Scotia shelf waters have a reduced buffering capacity because of significant freshwater input, making the region’s waters potentially more vulnerable to coastal acidification. Nutrient loading and heavy precipitation events further acid...

  11. A Comprehensive Review of Nova-Like Variable Stars

    Science.gov (United States)

    Sion, Edward

    2016-07-01

    A comprehensive review of nova-like variable stars of the VY Sculptoris and UX Ursa Majoris subtypes is presented. All that has been learned, up to the present time, from observations in the X-ray, far ultraviolet, optical and infrared bandpasses will be discussed. Spectroscopic analyses of high optical brightness states and low optical brightness states of nova-like variables will be summarized. The application of standard and non-standard accretion disk models as well as boundary layer structure will be discussed. The results of searches for nova shells, the evolutionary state of nova-likes as well as new spectroscopic results on BZ Cam (the bow shock CV) and BB Dor will also be included. This work is supported by NASA ADP grants NNX13AF12G and NNX13AF11G to Villanova University.

  12. The Place of Recurrent Novae among the Symbiotic Stars

    CERN Document Server

    Mikolajewska, Joanna

    2008-01-01

    The observational properties of recurrent novae indicate that they can be divided into two subclasses:systems with a dwarf and a red giant secondary, respectively. The second type -- which includes RS Oph -- bears many similarities to symbiotic stars.

  13. Quark nova inside supernova: Application to GRBs and XROs

    CERN Document Server

    Staff, Jan

    2010-01-01

    In this paper we consider a quark nova occurring inside an exploding star. The quark nova ejecta will shock when interacting with the stellar envelope. When this shock reaches the surface of the star, the energy is radiated away. We suggest that this energy may be seen in X-rays, and show here that this may explain some flares seen in the X-ray afterglow of long gamma ray bursts (GRBs). A quark nova inside an exploding star need not be followed by a GRB, or the GRB may not be beamed towards us. However, the shock breakout is likely not beamed and could be seen even in the absence of a GRB. We suggest that XRO 080109 is such an event in which a quark nova occurs inside an exploding star. No GRB is formed, but the break out of the shock leads to the XRO.

  14. AAS Nova and Astrobites: Making current astronomy research accessible

    Science.gov (United States)

    Kohler, Susanna; Astrobites Team

    2016-10-01

    AAS Nova and Astrobites are two resources available for astronomers, astronomy students, and astronomy enthusiasts to keep up with some of the most recent research published across the field of astronomy. Both supported by the AAS, these two daily astrophysical literature blogs provide accessible summaries of recent publications on the arXiv and in AAS journals. We present the goals, content, and readership of AAS Nova and Astrobites, and discuss how they might be used as tools in the undergraduate classroom.

  15. Synthesis of C-rich dust in CO nova outbursts

    Science.gov (United States)

    José, Jordi; Halabi, Ghina M.; El Eid, Mounib F.

    2016-09-01

    Context. Classical novae are thermonuclear explosions that take place in the envelopes of accreting white dwarfs in stellar binary systems. The material transferred onto the white dwarf piles up under degenerate conditions, driving a thermonuclear runaway. In these outbursts, about 10-7-10-3 M⊙, enriched in CNO and sometimes other intermediate-mass elements (e.g., Ne, Na, Mg, or Al for ONe novae) are ejected into the interstellar medium. The large concentrations of metals spectroscopically inferred in the nova ejecta reveal that the solar-like material transferred from the secondary mixes with the outermost layers of the underlying white dwarf. Aims: Most theoretical models of nova outbursts reported to date yield, on average, outflows characterized by O > C, from which, in principle, only oxidized condensates (e.g., O-rich grains) would be expected. Methods: To specifically address whether CO novae can actually produce C-rich dust, six different hydrodynamic nova models have been evolved, from accretion to the expansion and ejection stages, with different choices for the composition of the substrate with which the solar-like accreted material mixes. Updated chemical profiles inside the H-exhausted core have been used, based on stellar evolution calculations for a progenitor of 8 M⊙ through H- and He-burning phases. Results: We show that these profiles lead to C-rich ejecta after the nova outburst. This extends the possible contribution of novae to the inventory of presolar grains identified in meteorites, particularly in a number of carbonaceous phases (i.e., nanodiamonds, silicon carbides, and graphites).

  16. Synthesis of C-rich dust in CO nova ourbursts

    CERN Document Server

    Jose, Jordi; Eid, Mounib F El

    2016-01-01

    Context. Classical novae are thermonuclear explosions that take place in the envelopes of accreting white dwarfs in stellar binary systems. The material transferred onto the white dwarf piles up under degenerate conditions, driving a thermonuclear runaway. In those outbursts, about 10-7 - 10-3 Msun, enriched in CNO and, sometimes, other intermediate-mass elements (e.g., Ne, Na, Mg, or Al, for ONe novae) are ejected into the interstellar medium. The large concentrations of metals spectroscopically inferred in the nova ejecta reveal that the (solar-like) material transferred from the secondary mixes with the outermost layers of the underlying white dwarf. Aims. Most theoretical models of nova outbursts reported to date yield, on average, outflows characterized by O > C, from which only oxidized condensates (e.g, O-rich grains) would be expected, in principle. Methods. To specifically address whether CO novae can actually produce C-rich dust, six different hydrodynamic nova models have been evolved, from accreti...

  17. Early weaning and concentrate supplementation on slaughter weight and carcass characteristics of lambs produced on pasture Desmame precoce e a suplementação concentrada no peso ao abate e nas características de carcaça de cordeiros terminados em pastagem

    Directory of Open Access Journals (Sweden)

    Damaris Ferreira de Souza

    2011-06-01

    Full Text Available The study was designed to investigate the effect of early weaning and concentrate supplementation on the slaughter weight and carcass traits of Suffolk lambs in four production systems on Tifton-85 pasture: (1 suckling lambs not supplemented until slaughter; (2 suckling lambs supplemented with concentrate in creep feeders until slaughter; (3 early weaned lambs not supplemented until slaughter; (4 early weaned lambs supplemented with concentrate until slaughter. Lambs supplemented in creep feeding showed higher slaughter and carcass weights. Early weaning led to decrease and concentrate supplementation to increase in the yield and thickness of covering fat in the carcass, and the scores in pelvic-renal fat deposition, fat covering carcass and body condition to slaughter. Systems with early weaning and concentrate supplementation, and without weaning and supplementation allows that lambs reach suitable weight and body condition score to slaughter, resulting in production of carcasses with acceptable characteristics for marketing. Concentrate supplementation offered in creep feeders is useful to produce higher weight carcasses than those produced in systems with early weaning and concentrate supplementation, and without weaning and supplementation. The use of early weaning as a single strategy to produce lambs in pasture leads to unsuitable weight and body condition score to slaughter and is not recommended.Objetivou-se avaliar a influência das estratégias de desmame precoce e de suplementação concentrada no peso ao abate e nas características de carcaça de cordeiros Suffolk em quatro sistemas de terminação em pastagem de Tifton-85: (1 cordeiros mantidos ao pé da mãe e não suplementados até o abate; (2 cordeiros mantidos ao pé da mãe e suplementados com concentrado em creep feeding até o abate; (3 cordeiros desmamados precocemente e não suplementados até o abate; (4 cordeiros desmamados precocemente e suplementados com concentrado

  18. Another neon nova - Early infrared photometry and spectroscopy of Nova Cygni 1992

    Science.gov (United States)

    Hayward, T. L.; Gehrz, R. D.; Miles, J. W.; Houck, J. R.

    1992-01-01

    Infrared photometry and spectrophotometry of Nova Cygni 1992 taken within 54 days of its eruption show a strong 12.8-micron Ne II forbidden emission line as well as hydrogen recombination lines. Spectra with lambda/Delta lambda of about 2000 resolve the Ne II forbidden and 12.37-micron Hu-alpha lines with about 2200 km/s (FWHM). The Ne II forbidden line shows multiple velocity components. The amount of forbidden Ne II required to produce the observed emission feature exceeds the solar abundance of neon by at least a factor of 4.

  19. T Pyxidis: Death by a Thousand Novae

    CERN Document Server

    Patterson, Joseph; Kemp, Jonathan; Monard, Berto; Rea, Robert; Hambsch, Franz-Josef; McCormick, Jennie; Nelson, Peter; Allen, William; Krajci, Thomas; Lowther, Simon; Dvorak, Shawn; Borgman, Jordan; Richards, Thomas; Myers, Gordon; Harlingten, Caisey; Bolt, Greg

    2016-01-01

    We report a 20-year campaign to track the 1.8 hour photometric wave in the recurrent nova T Pyxidis, using the global telescope network of the Center for Backyard Astrophysics. During 1996-2011, that wave was highly stable in amplitude and waveform, resembling the orbital wave commonly seen in supersoft binaries. The period, however, was found to increase on a timescale P/P-dot=3x10^5 years. This suggests a mass transfer rate in quiescence of ~10^-7 M_sol/yr, in substantial agreement with the accretion rate based on the star's luminosity. This is ~2000x greater than is typical for cataclysmic variables of that orbital period. During the post-eruption quiescence (2012-2016), the star continued on its merry but mysterious way - similar luminosity, similar P/P-dot (2.4x10^5 years). The orbital signal became vanishingly weak (300 years of accretion at the pre-outburst rate, but the time between outbursts was only 45 years. Thus the erupting white dwarf seems to have ejected at least 6x more mass than it accreted....

  20. On Heavy Element Enrichment in Classical Novae

    CERN Document Server

    Alexakis, A; Heger, A; Brown, E F; Dursi, L J; Truran, J W; Rosner, R; Lamb, D Q; Timmes, F X; Fryxell, B; Zingale, M A; Ricker, P M; Olson, K

    2004-01-01

    Many classical nova ejecta are enriched in CNO and Ne. Rosner et al. recently suggested that the enrichment might originate in the resonant interaction between large-scale shear flows in the accreted H/He envelope and gravity waves at the interface between the envelope and the underlying C/O white dwarf. The shear flow amplifies the waves, which eventually form cusps and break. This wave breaking injects a spray of C/O into the superincumbent H/He. Using two-dimensional simulations, we formulate a quantitative expression for the amount of C/O that can be entrained into the H/He at saturation. The fraction of the envelope that is enriched depends on the shear velocity and density contrast between the C/O white dwarf and the H/He layer but is roughly independent of the shape of the shear profile. Using this parameterization for the mixed mass, we then perform several one-dimensional Lagrangian calculations of an accreting white dwarf envelope and consider two scenarios: that the wave breaking and mixing is driv...

  1. T Pyxidis: death by a thousand novae

    Science.gov (United States)

    Patterson, Joseph; Oksanen, Arto; Kemp, Jonathan; Monard, Berto; Rea, Robert; Hambsch, Franz-Josef; McCormick, Jennie; Nelson, Peter; Allen, William; Krajci, Thomas; Lowther, Simon; Dvorak, Shawn; Borgman, Jordan; Richards, Thomas; Myers, Gordon; Harlingten, Caisey; Bolt, Greg

    2017-04-01

    We report a 20-yr campaign to track the 1.8 h photometric (and orbital) wave in the recurrent nova T Pyxidis. Before and after the 2011 eruption, the period increased on a time-scale P/dot{P} = 3 × 105 yr. This suggests a mass transfer rate in quiescence of ˜10-7 M⊙ yr-1, in substantial agreement with the accretion rate based on the star's luminosity. During the eruption itself, a rapid period increase of 0.0054(7) per cent occurred. This is probably a measure of the mass ejected in the outburst. For a plausible choice of binary parameters, that mass is at least 3 × 10-5 M⊙, and probably more. This represents >300 yr of accretion at the pre-outburst rate, but the time between outbursts was only 45 yr. Thus, the erupting white dwarf (WD) seems to have ejected at least six times more mass than it accreted. If this eruption is typical, the WD must be eroding, rather than growing, in mass. Unless the present series of eruptions is a short-lived episode, the binary dynamics will evaporate the secondary in ˜105 yr. This could be a major channel by which short-period cataclysmic variables are removed from the population.

  2. Carnaval da Nova Consciência

    Directory of Open Access Journals (Sweden)

    Elisete Schwade

    2011-06-01

    Full Text Available Neste artigo faço uma descrição etnográfica do "Encontro Para a Nova Consciência" - ENC, que acontece anualmente em Campina Grande-PB, no período do carnaval, desde 1992. Um evento que promove o contato inter-religioso, ao mesmo tempo em que divulga uma "leitura" de realidades com conotação terapêutica. Propõe o diálogo de práticas religiosas com temas de amplo interesse na atualidade, tais como tolerância, paz, diversidade, questões ambientais, entre outros. Um espaço aberto que incorpora a cada edição novos diálogos, o que contribui para sua permanência. O texto sublinha interações e diálogos entre atores no ENC, por meio de referências associadas à religiosidade, enquanto vivência e partilha, num horizonte de produção e difusão de práticas e conteúdos que ganham expressividade pelo reconhecimento coletivo.

  3. Comportamento ingestivo de cordeiros em três sistemas de produção em pastagem de Tifton 85 - DOI: 10.4025/actascianimsci.v31i3.6014 Intake behavior of lambs in three production systems on Tifton 85 pasture - DOI: 10.4025/actascianimsci.v31i3.6014

    Directory of Open Access Journals (Sweden)

    Sergio Rodrigo Fernandes

    2009-09-01

    Full Text Available O objetivo deste estudo foi avaliar o comportamento ingestivo de cordeiros em pastagem de Tifton-85 (Cynodon spp. em três sistemas de produção: cordeiros desmamados aos 60 dias de idade e mantidos em pastagem; cordeiros mantidos com suas mães em pastagem; e cordeiros mantidos com suas mães em pastagem e suplementados em creep feeding. O delineamento foi em blocos ao acaso com três repetições, utilizando quatro cordeiros-teste por repetição. Na pastagem, avaliou-se a altura, a massa, a composição morfológica e bromatológica da forragem. Na avaliação do comportamento ingestivo registrou-se, do nascer ao pôr do sol, o tempo despendido nas atividades de pastejo, ruminação, ócio, amamentação e alimentação no creep feeding. Avaliou-se, também, a taxa de bocados ao pastejo. Os cordeiros permaneceram maior tempo em pastejo, e os suplementados despenderam menor (p creep feeding alterou (p The objective of this study was to evaluate the intake behavior of lambs on Tifton 85 pasture (Cynodon spp. in three production systems: sixty-days-old weaned lambs kept on pasture; lambs kept with their mother on pasture; lambs kept with their mother on pasture in creep feeding. Systems were allocated in a completely randomized blocks design with three replicates and four lambs per replicate. Pasture sward surface height, forage dry matter, and morphological and nutritional characters were assessed. Intake behavior was observed from dawn to dusk. The study assessed the time animals spent in the following activities: grazing, ruminating, idling, suckling, and staying in creep feeding. Bite rate was also evaluated. Lambs spent most of their time grazing, but the supplemented ones spent less time (p creep feeding altered (p < 0.05 distribution of grazing and rumination, indicating a substitutive effect of pasture by concentrate. Sheep production systems affected the intake behavior of lambs, but did not affect the bite rate.

  4. ATIVIDADE ANTI-HELMÍNITICA DO TRICLORFOM E CLOSANTEL EM CORDEIROS NATURALMENTE INFECTADOS POR HAEMONCHUS SP ANTHELMINTICS ACTIVITY TRICLORFOM AND CLOSANTEL IN THE LAMBS NATURALLY INFECTED WITH HAEMONCHUS SP

    Directory of Open Access Journals (Sweden)

    Margarete Kimie Falbo

    2009-09-01

    Full Text Available

    Este trabalho teve como objetivo avaliar a atividade anti-helmíntica do triclorfon (Neguvon® e closantel (Zuletel® em cordeiros naturalmente infectados com Haemonchus sp. Constituíram-se três grupos de nove cordeiros cada, mestiços Ile de France com Corriedale, com noventa dias de idade. No Grupo 1, os animais foram medicados com triclorfon (Neguvon®, por via oral na dose de 97 mg.kg-1 de peso vivo; no Grupo 2, a medicação utilizada foi closantel (Zuletel® na dose de 10 mg.kg-1 peso vivo; no Grupo 3, os animais não receberam nenhum tipo de tratamento anti-helmintico. Por meio do teste de redução da OPG, constatou-se que o triclorfon apresentou eficácia de 97,9% e o closantel 55,2%. Registra-se pela primeira vez resistência ao closantel em cordeiros na área central do estado do Paraná, Brasil.
     
    PALAVRAS-CHAVES: Closantel, Haemonchus sp, ovinos, triclorfon.

    This study aimed to evaluate the activity of anthelmintic trichlorfon (Neguvon ® and closantel (Zuletel ® in lambs naturally infected with Haemonchus sp. Twenty-seven lambs, crossbred Ile of France with Corridale, 90 days-old, were divided into 3 groups of nine animals: Group 1, animals were treated with trichlorfon (Neguvon ® orally at a dose of 97 mg.kg-1 body weight, Group 2 were treated with closantel (Zuletel ® at a dose of 10 mg .kg-1 body weight and Group 3 did not receive any kind of anthelmintic treatment. Through the test of reduction of OPG could be noted that the trichlorfon showed effectiveness of 97.9% and 55.2% closantel. It is noted the first closantel resistance in lambs in the central area of the state of Parana, Brazil.

    KEY WORDS: Closantel, Haemonchus sp, sheep, triclorfon

  5. Características de carcaça de cordeiros alimentados com grãos e subprodutos da canola = Carcass characteristics in lambs fed with grains and by-products of canola

    Directory of Open Access Journals (Sweden)

    José Carlos Barbosa

    2009-10-01

    Full Text Available O objetivo foi estudar a introdução de 8% de grãos e subprodutos (farelo ou torta da canola em dietas para cordeiros. Para a avaliação das características quantitativas da carcaça, foram utilizadas 24 carcaças de cordeiros, utilizando delineamento inteiramente casualizado. As dietas com média de 15,4% de PB na MS e 80,2% de NDT foram compostas por 40% de feno de capim-Tifton e 60% de concentrado composto por milho em grão, farelo de soja, canola em grão integral, farelo de canola, torta de canola e mistura mineral. A utilização de grãos e subprodutos da canola na dieta de borregos terminados em confinamento não influenciou (p > 0,05 as características quantitativas da carcaça. Em relação aos rendimentos dos cortes, não houve efeito dos tratamentos para nenhuma das variáveis analisadas. Assim, a introdução de 8% de grãos e subprodutos (farelo ou torta da canola possibilitaram bons resultados podendo ser recomendados nas formulações de dietas para cordeiros.The aim of this work was to evaluate the introduction of 8% grains and by-products (meal or cake of canola in the diets of lambs. To evaluate quantitative carcass characteristics, 24 Santa Ines lambs were used in a completely randomized design. Diets with averages of 15.4% of CP in DM and 80.2% of TDN were composed for 40% Tifton hay and 60% concentrate based on corn grain, soybean meal, whole grain canola, canola meal, canola cake and mineral mixture. The use of whole grains and by-products of canola in the diet of lambs finished in feedlot did not influence (p > 0.05 quantitative carcass characteristics. For cut dressing in relation to the CCW, no effect was observed for the analyzed variables among treatments. It was concluded that the introduction of grains and by-products of canola allow for satisfactory results, and could be recommended in the formulations of lamb diets.

  6. Outburst of the recurrent nova V745 Sco

    Science.gov (United States)

    Waagen, Elizabeth O.

    2014-02-01

    The outburst of the recurrent nova V745 Sco (Nova Sco 1937) by Rod Stubbings (Tetoora Road, VIC, Australia) at visual magnitude 9.0 on 2014 February 6.694 UT is reported. This recurrent nova is fading quickly. Follow-up observations of all types (visual, CCD, DSLR) are strongly encouraged, as is spectroscopy; fast time-series of this nova may be useful to detect possible flaring activity as was observed during the outburst of U Scorpii in 2010. Coincident time-series by multiple observers would be most useful for such a study, with a V-filter being preferred. Observations reported to the AAVSO International Database show V745 Sco at visual mag. 10.2 on 2014 Feb. 07.85833 UT (A. Pearce, Nedlands, W. Australia). Finder charts with sequence may be created using the AAVSO Variable Star Plotter (http://www.aavso.org/vsp). Observations should be submitted to the AAVSO International Database. Previous outbursts occurred in 1937 and 1989. The 1937 outburst was detected in 1958 (in decline at magnitude 11.0 on 1937 May 11.1 UT; outburst had occurred within the previous 19 days) by Lukas Plaut on plates taken by Hendrik van Gent at the Leiden Observatory; the object was announced as Nova Sco 1937 and later assigned the GCVS name V745 Sco. The 1989 outburst was detected on 1989 August 1.55 UT by Mati Morel (MMAT, Thornton, NSW, Australia) at visual magnitude 10.4 and in decline. Dr. Bradley Schaefer (Louisiana State University) reports (2010ApJS..187..275S) in his comprehensive analysis of the 10 known galactic recurrent novae (including V745 Sco) that the median interval between recurrent novae outbursts is 24 years. The interval since the 1989 outburst of V745 Sco is 24.10 years. See the Alert Notice for additional visual and multicolor photometry and for more details.

  7. Terra Nova Environmental effects monitoring program

    Energy Technology Data Exchange (ETDEWEB)

    Williams, U. [Petro-Canada Inc., St. John' s, NF (Canada); Murdoch, M. [Jacques Whitford Environmental Limited (Canada)

    2000-07-01

    Elements of the environmental effects monitoring program in the Terra Nova oil field, about 350 km east-southeast of St. John's, Newfoundland, are described. This oilfield is being developed using a floating production storage and offloading (FPSO) facility. A total of 24 wells are expected to be drilled through seven subsea templates located in four glory holes to protect them from icebergs. Subsea installations will be linked to the FPSO by trenched flowlines connected to flexible risers. The FPSO will offload to shuttle tankers. First oil is expected in 2001. The environmental effects monitoring program will be conducted annually for the first two years beginning in 2000. Subsequent scheduling will be determined after a review of monitoring data collected during the first three years. Input to the design of the monitoring program was provided by all stakeholders, i. e. owners, local public, government agencies and regional and international experts. A model was developed linking project discharges and possible effects to the environment, including marine resources in the area, and the information derived from these activities was used to generate a set of predictions and hypotheses to be tested in the monitoring program. The monitoring program will use two spatial models: a regression or gradient design and a control-impact design. The gradient design will monitor water column and sediment chemistry, sediment toxicity and benthic invertebrate communities. The control-impact design will be used to monitor larger and more mobile fish or shellfish. The evaluated results will serve as the basis for determining impact predictions and to provide information to allow for decisions pertaining to the protection of the marine environment.

  8. Massive NLTE models for X-ray novae with PHOENIX

    CERN Document Server

    van Rossum, Daniel R

    2012-01-01

    X-ray grating spectra provide the confirmation of continued mass loss from novae in the super-soft source (SSS) phase of the outburst. In this work expanding nova atmosphere models are developed and used to study the effect of mass loss on the SSS spectra. The very high temperatures combined with high expansion velocities and large radial extension make nova in the SSS phase very interesting but also difficult objects to model. The radiation transport code PHOENIX was applied to SSS novae before, but careful analysis of the old results has revealed a number of problems which lead to new methods and improvements to the code: 1) an improved NLTE module (a new opacity formalism, rate matrix solver, global iteration scheme, and temperature correction method); 2) a new hybrid hydrostatic-dynamic nova atmosphere setup; 3) the models are treated in pure NLTE (no LTE approximation for any opacity). With the new framework a modest amount of models (limited by computation time) are calculated. These show: 1) systematic...

  9. π0 mass reconstruction in NOvA Far Detector.

    Science.gov (United States)

    Edayath, Sijith

    2017-01-01

    NOvA is a long-baseline neutrino oscillation experiment with functionally identical, segmented, tracking calorimeter Near and Far detectors. The detectors lie 14.6 mrad off-axis from the Fermilab NuMI beam, with a well-defined peak in neutrino energy at 2 GeV. The absolute calibration of the energy scale of the detectors is a major systematic uncertainty in long-baseline oscillation search in NOvA. Neutrino detectors make use of some standard candles for absolute energy calibration. Stopping muon energy distributions, Michel electron energy distributions, and invariant π0 mass are among them. In this talk, we cover NOvA's use of a new method to identify π0 with cosmic origins in the NOvA Far Detector. We employ a computer vision based particle identifier using convolutional neural networks (CVN) to identify π0s, complementing an existing strategy to identify π0 from the neutrino beam using more traditional methods in the Near Detector. Registered for PhD at Cochin University of Science and Technology, India and doing research in NOvA experiment at Fermilab.

  10. Fermi Reveals New Light on Novae in Gamma rays

    CERN Document Server

    Cheung, C C; Shore, S N; Grove, J E; Leising, M

    2016-01-01

    Novae are now firmly established as a high-energy (>100 MeV) gamma-ray source class by the Fermi Large Area Telescope (LAT). In symbiotic binary systems such as V407 Cyg 2010, there is a firm theoretical framework for the production of shock-accelerated particles in the nova ejecta from interactions with the dense wind of the red giant companion. Yet, the high-energy gamma-ray emission detected in classical novae involving less evolved stellar companions cannot be explained in the same way and could instead be produced in internal shocks in the ejecta. We summarize the Fermi-LAT gamma-ray observations of novae, highlighting the main properties that will guide further studies. Additionally, we report on the soft gamma-ray (~0.1 MeV) continuum detection of the oxygen-neon type classical nova V382 Vel 1999 with the OSSE detector aboard the Compton Gamma Ray Observatory in light of its Fermi-era analog, V959 Mon 2012.

  11. Avaliação sensorial da carne de cordeiros machos e fêmeas Texel × Corriedale terminados em diferentes sistemas Sensory evaluation of meat lambs from males and femeles Texel × Corriedale finished in different systems

    Directory of Open Access Journals (Sweden)

    Marlice Salete Bonacina

    2011-08-01

    Full Text Available O objetivo neste trabalho foi avaliar o efeito do sexo e de três sistemas de terminação nas características sensoriais da carne de cordeiros Texel × Corriedale e na aceitação da carne pelo consumidor. Foram utilizados 90 animais, 45 cordeiros machos não-castrados e 45 fêmeas mantidos em pastagem até o desmame (70 dias e terminados em três sistemas de produção: pastagem; pastagem ao pé da mãe; e pastagem com suplementação (casca de soja em nível correspondente a 1% do peso vivo dos cordeiros. Após o abate, as carcaças foram armazenadas em câmara fria, com ar forçado, a 1ºC, durante 24 horas, para retirada do músculo longissimus dorsi, que foi congelado a -18ºC para análise sensorial. A caracterização sensorial da carne foi realizada por meio da análise descritiva quantitativa: 22 termos descritivos foram desenvolvidos por uma equipe de julgadores selecionados, que geraram também a definição de cada termo e as amostras-referência. Foi realizado um teste de aceitação utilizando escala hedônica híbrida de nove pontos. A carne dos machos e dos animais terminados em pastagem ao pé da mãe caracterizou-se pelo odor e sabor residual mais suaves de carne ovina e gordura, menor maciez e maior mastigabilidade em comparação à das fêmeas e dos animais terminados nos demais sistemas. As carnes dos cordeiros terminados nos sistemas de pastagem e de pastagem com suplementação são semelhantes quanto aos aspectos sensoriais. A carne é igualmente aceita pelos consumidores, independentemente do sexo e do sistema de terminação, apresentando boa aceitação.The objective of this work was to evaluate the effect of sex and of three finishing systems on sensory traits of Texel × Corriedale lamb meat an on the consumer acceptance of the meat. It was used 90 animals, 45 non-castrated male lambs and 45 females kept on pasture until weaning (70 days of age and finished in three production systems: pasture, pasture with mother

  12. Desempenho reprodutivo de ovelhas mestiças da raça Santa Inês em Brachiaria humidícula e efeito do sexo no ganho de peso de cordeiros

    Directory of Open Access Journals (Sweden)

    P.A. Oliveira

    2014-02-01

    Full Text Available Objetivou-se avaliar o desempenho reprodutivo de ovelhas deslanadas em função do manejo alimentar das crias e idade de desmame, além de mensurar o efeito do sexo no ganho de peso de cordeiros. Sessenta e quatro ovelhas mestiças da raça Santa Inês foram distribuídas em delineamento inteiramente ao acaso, em esquema fatorial 4 x 2 x 2 - quatro idades de desmame (56, 70, 84 e 98 dias, sexo e manejo alimentar das crias, cada tratamento com quatro repetições. As ovelhas foram manejadas com a cria ao pé, em 14 piquetes de 1,5 ou 2,0 hectares, formados com pastagem de Brachiaria humidícola. As crias nascidas de partos simples, filhos de reprodutores Santa Inês puros de origem (PO. Após o desmame de todos os grupos, sessenta e quatro cordeiros (32 machos e 32 fêmeas foram distribuídos ao acaso em baias individuais e confinados por 30 dias. A comparação dos parâmetros foi realizada pelo ajuste do modelo de regressão linear simples. Verificou-se vício de tempo longo do manejo alimentar das crias de + 3,7% (P<0,05 para o intervalo entre partos e de + 1,4% (P<0,05 para o período de serviço. Houve efeito linear crescente (P<0,05 da idade de desmame sobre o intervalo entre partos e período de serviço. Verificou-se vício de tempo longo do sexo das crias de + 2,0% (P<0,05 para o intervalo entre partos e de + 0,8% (P<0,05 para o período de serviço das ovelhas. Constatou-se vício de tempo longo do sexo de + 35,2% e + 36,9% (P<0,05, respectivamente, para o ganho de peso diário de cordeiros do nascimento ao desmame e pós desmame em confinamento. A suplementação das crias em alimentador privativo e a antecipação da idade de desmame reduzem o intervalo entre partos e período de serviço de ovelhas deslanadas em pastagem de Brachiaria humidícula. O sexo da cria é fonte de variação na análise da eficiência reprodutiva de matrizes ovinas e no ganho de peso de cordeiros mestiços da raça Santa Inês do nascimento ao desmame e ap

  13. Anthelmintic activity of Melia azedarach fruits in lambs naturally infected with gastrointestinal nematodes / Atividade anti-helmíntica do fruto da Melia azedarach em cordeiros naturalmente infectados com nematódeos gastrintestinais

    Directory of Open Access Journals (Sweden)

    Daniela Guzzo

    2008-08-01

    Full Text Available The aim of this study was to evaluate the anthelmintic activity of Melia azedarach grounded dry fruits, in lambs naturally infected with gastrointestinal nematodes. Twenty four (24 mixed-breed Ile de France x Corriedale, male lambs, aged 3 month, were separeted into three (3 groups of eight (8 animals: the first group was medicated with 5mg.Kg-1 of albendazole orally, in a single dose, the second group was medicated with 2g.Kg-1 of Melia azedarach fruits orally, in a single dose, and the third group remained untreated, as control. The results showed that the group that presented the best efficacy was the one treated with albendazole (51.96%, followed by the group treated with Melia azedarach fruits that presented 33.21% of efficacy.Objetivou-se neste trabalho avaliar a atividade anti-helmíntica dos frutos secos e moídos da planta Melia azedarach, em cordeiros naturalmente infectados com nematódeos gastrintestinais. Utilizou-se 24 cordeiros, com 90 dias de idade, machos, mestiços Ile de France x Corridale, os quais foram divididos em 3 grupos de oito animais cada, sendo: grupo 1, medicado com 5mg.Kg-1 em dose única, de albendazole pela via oral (V.O; grupo 2, com 2g.Kg-1 (V.O, em dose única, do fruto do cinamomo (Melia azedarach e o grupo 3, controle, não recebeu nenhum tipo de tratamento. Os resultados encontrados demonstraram que o grupo tratado com albendazole foi o que apresentou melhor eficácia 51.96%, seguido do grupo tratado com frutos de cinamomo o qual apresentou eficácia de 33.21%.

  14. Desempenho e características de carcaça de cordeiros Suffolk alimentados com diferentes volumosos Performance and carcass traits of Suffolk lambs fed with different roughages

    Directory of Open Access Journals (Sweden)

    Eduardo Antonio da Cunha

    2001-08-01

    Full Text Available Cordeiros da raça Suffolk, desmamados aos 60 dias e confinados, foram alimentados com silagem de milho, silagem de sorgo granífero ou feno de Coast cross (Cynodon dactylon L. Pears e ração concentrada (3,5% do peso vivo, com o objetivo de avaliar seu desempenho, a proporção dos componentes-não-carcaça e o rendimento e características das suas carcaças. Foi utilizado um delineamento completamente casualizado em esquema fatorial (três alimentos volumosos e dois sexos. Os animais alimentados com silagem de milho ou de sorgo mostraram maior (P0,05 pelo tipo de alimento, contudo, os animais alimentados com silagem de milho apresentaram carcaças com maior (P0,05 na proporção de músculos (60,0 e 60,7%. A silagem de sorgo pode substituir a silagem de milho para cordeiros confinados, contudo o uso do feno de gramínea reduz o seu desempenho.Suffolk lambs, weaned at 60 days, were raised in slatted floor pens and fed corn silage, sorghum silage or Coast cross hay (Cynodon dactylon L. Pears plus concentrate ration (3,5% of live weight to evaluate their performance, proportion of non-carcass components and carcass dressing and traits. A completely randomized design in a factorial arrangement (tree roughage feed X two sexes was used. Lambs fed corn silage or sorghum silage showed greater (P0.05 between feeds, although, lambs fed corn silage showed greater (P0.05 in proportion of muscle (60.0 and 60.7%. Sorghum silage can replace corn silage for feedlot lambs, but grass hay feeding worsens their performance.

  15. Consumo alimentar residual e sua relação com medidas de desempenho e eficiência e características in vivo da carcaça de cordeiros

    Directory of Open Access Journals (Sweden)

    E.F.E. Paula

    2013-04-01

    Full Text Available Avaliou-se o consumo alimentar residual (CAR e a conversão alimentar (CA de 20 cordeiros, com o objetivo de estimar as correlações entre essas variáveis com medidas de desempenho e com características in vivo da carcaça. Os animais tiveram o consumo de MS (CMS mensurado por 65 dias e foram pesados a cada 13 dias para obtenção do ganho médio diário (GMD. Foram considerados o peso vivo inicial (PVI, o peso vivo final (PVF, o peso metabólico (PM, o GMD, a taxa de crescimento relativo (TCR, a taxa de Kleiber (TK, a CA, o CMS e o CMS em percentual do PV (CMSPV. As avaliações de carcaça foram realizadas por ultrassom. O CAR se mostrou correlacionado com o CMS (+0,81, o CMSPV (+0,90 e a CA (+0,63. Correlações significativas foram encontradas entre CA e GMD; CA e TCR; CA e TK; e CA e PVI (-0,63, -0,74, -0,75 e +0,51, respectivamente. O CAR e a CA não se mostraram correlacionados com características de carcaça, e, da mesma forma, não houve diferença entre as classes de CAR para essas variáveis. Confirmou-se o potencial do CAR como medida de eficiência alimentar para cordeiros em confinamento, sem existência de relações com o ganho de peso e o tamanho corporal e sem alterações na composição da carcaça.

  16. Análise econômica da produção de carne de cordeiros sob dois sistemas de terminação: pastagem e confinamento Economical analysis of meat lamb production under two finishing systems: pasture and dry-lot

    Directory of Open Access Journals (Sweden)

    Francisco de Assis Fonseca de Macedo

    2000-08-01

    Full Text Available Foram analisados os custos de produção e o retorno econômico do quilograma de carcaça, de 13 cordeiros Corriedale (C, 14 Bergamácia x Corriedale (BC e 9 Hampshire Down x Corriedale (HC, em pastagem de Cynodon dactylon e 10 C, 11 BC e 8 HC em confinamento, recebendo ração completa, com 18% de proteína bruta e 72% de nutrientes digestíveis totais, idênticos ao da pastagem. A lotação utilizada foi de 20 cordeiros/ha. No confinamento, considerou-se 0,5m²/cordeiro. A despesa total para terminação dos cordeiros na pastagem foi R$2.382,40 e para terminação em confinamento foi R$2.918,40, com as respectivas receitas de R$3.686,90 e R$4.498,03. O custo de produção do kg de carcaça dos cordeiros confinados (R$2,30, em valor absoluto foi superior, porém, muito próximo dos terminados em pastagem (R$2,26. O retomo econômico para os cordeiros terminados em confinamento (R$1.579,63 foi superior ao dos terminados em pastagem (R$1.304,50, mostrando uma diferença em valores absolutos de R$275,13 a favor dos cordeiros confinados. A produção de carne de cordeiro em confinamento é economicamente viável.This experiment was carried out to study costs and economical return of carcass lamb (kg production in two finishing systems. The systems compared were, a grazing system based on "coast cross" pasture (Cynodon dactylon with the following genotypes: 13 Corriedale (C. 14 Bergamacia x Corriedale (BC, and 9 Hampshire Down x Corriedale {HC}, and a dry-lot system with the following crossbreeds : 10 C, 11 BC, and 8 HC. In the dry-lot system the lambs were fed with a total mix ration, containing the some leveis ofcrude protein and total digestible nutrients of the pasture. The stock rate in the pasture was 20 lambs/ha. In the dry-lot was used an área of 0.5m²/lamb and the lambs were housed in a suspenso and siated floor facitity. The total costs in the graang system was US$ 1985.33, and in the dry-lot system was US$ 2432.00. The total incarne for

  17. Aspectos ambientais, produtivos e econômicos do aproveitamento de resíduo úmido de cervejaria na alimentação de cordeiros em sistema de confinamento Environmental, productive and economic aspects of use of brewery residue as food of lamb feedlots in finishing phase

    OpenAIRE

    Mariana Augusta Brochier; Sérgio Carvalho

    2009-01-01

    Objetivou-se com este trabalho avaliar a geração e o poder poluente do resíduo úmido de cervejaria e determinar aspectos produtivos e a economicidade do uso desse resíduo em substituição ao alimento concentrado na alimentação de cordeiros confinados em fase de terminação. Foram utilizados 25 cordeiros, machos, não-castrados, da raça Texel, oriundos de parto simples, desmamados aos 69 dias de idade em média. Foram avaliados cinco níveis de substituição do alimento concentrado por resíduo úmido...

  18. The Star of Bethlehem is Not the Nova DO Aquilae (Nor Any Other Nova, Supernova, or Comet)

    CERN Document Server

    Schaefer, Bradley E

    2013-01-01

    The Star of Bethlehem is only known from a few verses in the Gospel of Matthew, with the Star inspiring and leading the Magi (i.e., Persian astrologers) to Jerusalem and ultimately worshipping the young Jesus Christ in Bethlehem. In the last four centuries, astronomers have put forth over a dozen greatly different naturalistic explanations, all involving astronomical events, often a bright nova, supernova, or comet. This paper will evaluate one prominent recent proposal, that the Star was a 'recurrent nova' now catalogued as DO Aquilae, and provide three refutations. In particular, (1) DO Aql is certainly not a recurrent nova, but rather an ordinary nova with a recurrence time scale of over a million years, (2) in its 1925 eruption, DO Aql certainly never got brighter than 8.5 mag, and the physics of the system proves that it could never get to the required luminosity of a supernova, and (3) the Magi were astrologers who had no recognition or interpretation for novae (or supernovae or comets) so any such even...

  19. Nova KT Eri 2009: Infrared studies of a very fast and small amplitude He/N nova

    CERN Document Server

    Raj, Ashish; Ashok, N M

    2013-01-01

    We present near-infrared spectroscopic and photometric observations of the nova KT Eridani taken during the first 100 days following its discovery in 2009 November. The JHK spectra of the object have been taken from the Mount Abu Infrared Observatory using the Near-Infrared Imager/Spectrometer. The spectra, typical of the He/N class novae, show strong He I emission lines together with H I and O I emission features. The H I, Pa-beta and Br-gamma spectral lines and the He I line at 2.0581 micron show broad wings with a relatively narrow central component. The broad wings extend to 1900 km/s while the central component has FWHM of 2100 km/s. The V and near-infrared JHK light curves show an additional small amplitude outburst near 40 days after optical maximum. The distance to the nova d = 6.3 +/- 0.1 kpc is derived using the MMRD relation and the estimated value of t2 = 5.7 +/- 0.3 days. The small value of t2 places KT Eri in the class of very fast novae. Using the value of the distance to the nova d, we estimat...

  20. Very-high-energy {\\gamma}-ray observations of novae and dwarf novae with the MAGIC telescopes

    CERN Document Server

    Ahnen, M L; Antonelli, L A; Antoranz, P; Babic, A; Banerjee, B; Bangale, P; de Almeida, U Barres; Barrio, J A; González, J Becerra; Bednarek, W; Bernardini, E; Biasuzzi, B; Biland, A; Blanch, O; Bonnefoy, S; Bonnoli, G; Borracci, F; Bretz, T; Carmona, E; Carosi, A; Chatterjee, A; Clavero, R; Colin, P; Colombo, E; Contreras, J L; Cortina, J; Covino, S; Da Vela, P; Dazzi, F; De Angelis, A; De Caneva, G; De Lotto, B; Wilhelmi, E de Oña; Mendez, C Delgado; Di Pierro, F; Prester, D Dominis; Dorner, D; Doro, M; Einecke, S; Glawion, D Eisenacher; Elsaesser, D; Fernández-Barral, A; Fidalgo, D; Fonseca, M V; Font, L; Frantzen, K; Fruck, C; Galindo, D; López, R J García; Garczarczyk, M; Terrats, D Garrido; Gaug, M; Giammaria, P; Godinović, N; Muñoz, A González; Guberman, D; Hanabata, Y; Hayashida, M; Herrera, J; Hose, J; Hrupec, D; Hughes, G; Idec, W; Kellermann, H; Kodani, K; Konno, Y; Kubo, H; Kushida, J; La Barbera, A; Lelas, D; Lewandowska, N; Lindfors, E; Lombardi, S; Longo, F; López, M; López-Coto, R; López-Oramas, A; Lorenz, E; Majumdar, P; Makariev, M; Mallot, K; Maneva, G; Manganaro, M; Mannheim, K; Maraschi, L; Marcote, B; Mariotti, M; Martínez, M; Mazin, D; Menzel, U; Miranda, J M; Mirzoyan, R; Moralejo, A; Nakajima, D; Neustroev, V; Niedzwiecki, A; Rosillo, M Nievas; Nilsson, K; Nishijima, K; Noda, K; Orito, R; Overkemping, A; Paiano, S; Palacio, J; Palatiello, M; Paneque, D; Paoletti, R; Paredes, J M; Paredes-Fortuny, X; Persic, M; Poutanen, J; Moroni, P G Prada; Prandini, E; Puljak, I; Reinthal, R; Rhode, W; Ribó, M; Rico, J; Garcia, J Rodriguez; Saito, T; Saito, K; Satalecka, K; Scapin, V; Schultz, C; Schweizer, T; Sillanpää, A; Sitarek, J; Snidaric, I; Sobczynska, D; Stamerra, A; Steinbring, T; Strzys, M; Takalo, L; Takami, H; Tavecchio, F; Temnikov, P; Terzić, T; Tescaro, D; Teshima, M; Thaele, J; Torres, D F; Toyama, T; Treves, A; Verguilov, V; Vovk, I; Will, M; Zanin, R; Desiante, R; Hays, E

    2015-01-01

    Context. In the last five years the Fermi Large Area Telescope (LAT) instrument detected GeV {\\gamma}-ray emission from five novae. The GeV emission can be interpreted in terms of an inverse Compton process of electrons accelerated in a shock. In this case it is expected that protons in the same conditions can be accelerated to much higher energies. Consequently they may produce a second component in the {\\gamma}-ray spectrum at TeV energies. Aims. We aim to explore the very-high-energy domain to search for {\\gamma}-ray emission above 50 GeV and to shed light on the acceleration process of leptons and hadrons in nova explosions. Methods. We have performed observations with the MAGIC telescopes of the classical nova V339 Del shortly after the 2013 outburst, triggered by optical and subsequent GeV {\\gamma}-ray detec- tions. We also briefly report on VHE observations of the symbiotic nova YY Her and the dwarf nova ASASSN-13ax. We complement the TeV MAGIC observations with the analysis of con- temporaneous Fermi-...

  1. Ultrastructure of extrusomes in hypotrichous ciliate Pseudourostyla nova

    Institute of Scientific and Technical Information of China (English)

    ZHOU Yao; WANG Zhengjun; ZHANG Jun; GU Fukang

    2011-01-01

    The ultrastructure of extrusomes of the hypotrichous ciliate Pseudourostyla nova was observed in scanning and transmission electron microscopy and enzyme-cytochemistry. The results show that the distribution, morphological characteristics, morphogenesis process, and extrusive process of the extrusomes in P. nova are different from the trichocysts in Paramecium, suggesting that the extrusomes of P. nova can respond to environmental stimuli, play an important role in the defense of this species, and cannot be regarded as "trichocysts". The results also suggest that the extrusomes might be originated from the Golgi apparatus and mature in the cytoplasm; after the extrusion of mature extrusomes, the residual substance might be reabsorbed and reused by the ciliate cell via food vacuoles, and take part in material recycling of the cell.

  2. First Neutrino Oscillation Results from the NOvA experiment

    Energy Technology Data Exchange (ETDEWEB)

    Sachdev, Kanika [Fermilab

    2016-11-29

    NOvA is a long-baseline neutrino oscillation experiment on the NuMI muon neutrino beam at Fermilab. It consists of two functionally identical, nearly fully-active liquid-scintillator tracking calorimeters. The Near Detector (ND) at Fermilab is used to study the neutrino beam spectrum and composition before oscillations occur. The Far Detector in northern Minnesota, 810 km away, observes the oscillated beam and is used to extract the oscillation parameters. NOvA is designed to observe oscillations in two channels: disappearance channel ( ν μ → ν μ ) and ν e appearance channel ( ν μ → ν e ). This paper reports the measurements of both these channels based on the first NOvA data taken from February 16, 2014 till May 15, 2015

  3. Liquid scintillator production for the NOvA experiment

    CERN Document Server

    Mufson, S; Bower, C; Coan, T; Cooper, J; Corwin, L; Karty, J; Mason, P; Pla-Dalmau, A; Proudfoot, M

    2015-01-01

    The NOvA collaboration blended and delivered 8.8 kt (2.72M gal) of liquid scintillator to its detectors as its active detector medium. The composition of the scintillator was developed to meet the requirements of the experiment. The scintillator was shipped to the NOvA near and far detectors using dedicated stainless steel tanker trailers. A rigorous set of quality control procedures were put in place to assure that the liquid scintillator was blended to satisfy the transparency, light yield, and conductivity requirements. The incoming components, the blended scintillator, and the scintillator in the transport tanker trailers were all qualified with these procedures, which ensured that the NOvA scintillator was high quality and met its performance requirements.

  4. Desempenho e digestibilidade dos nutrientes em cordeiros alimentados com dietas contendo silagem de resíduos de peixe Performance and digestibility of nutrients in lambs fed diets containing fish residue silage

    Directory of Open Access Journals (Sweden)

    Sandra Mari Yamamoto

    2007-08-01

    Full Text Available Foram utilizados 36 cordeiros 7/8 Ile de France 1/8 Ideal (18 machos e 18 fêmeas com peso corporal inicial de 17,90 ± 1,27 kg alimentados com as dietas: controle; SRPAD - com 8% de silagem de resíduo do processamento de tilápia (Oreochromis niloticus; e SRPAM - com 8% de silagem de resíduo do processamento de peixe-sapo (Lophius gastrophisus. As silagens de resíduos de peixes substituíram parcialmente o farelo de soja e, como volumoso, utilizou-se silagem de milho (40%. Os cordeiros foram mantidos em baias individuais, com controle do alimento fornecido e das sobras e pesagem a cada 14 dias até atingirem 32 kg, quando foram realizadas as medidas biométricas. Paralelamente, foram realizados ensaios de digestibilidade e de metabolismo utilizando-se 12 cordeiras 7/8 Ile de France 1/8 Ideal para determinação dos coeficientes de digestibilidade da MS, MO, PB, EE, FDN e CT e do balanço de nitrogênio das dietas experimentais. O consumo de MS e o ganho médio diário não foram influenciados pelas dietas e pelo sexo e apresentaram médias de 891,83 e 240,26 g/dia, respectivamente. Entretanto, a conversão alimentar dos cordeiros alimentados com as dietas com SRPAM foi pior (4,04 em relação à daqueles alimentados com as dietas controle (3,81 e com SRPAD (3,47. Os cordeiros apresentaram maior comprimento corporal (60,09 cm e altura do anterior (56,11 cm em comparação às cordeiras (58,03 e 54,75 cm, respectivamente. Cordeiros alimentados com dietas contendo SRPAD tiveram maior ingestão de EE e melhor coeficiente de digestibilidade do EE (90,39%, enquanto aqueles alimentados com a dieta controle apresentaram o menor coeficiente de digestibilidade da FDN (59,20%. A substituição parcial do farelo de soja por silagem de resíduos de peixes mostrou-se como boa alternativa protéica na alimentação de cordeiros.Thirty six 7/8 Ile de France 1/8 Polwarth (18 males and 18 females lambs averaging 17.90 ± 1.27 kg of body weigh (BW were

  5. Influence of feeding regime and finishing system on lamb muscle fiber and meat quality Influência do regime alimentar e do sistema de terminação sobre as fibras musculares e a qualidade da carne de cordeiros

    Directory of Open Access Journals (Sweden)

    Sarita Bonagurio Gallo

    2009-11-01

    e a qualidade da carne dos cordeiros. Utilizaram-se matrizes mestiças Ile de France × Bergamacia criadas a pasto. As ovelhas foram divididas em dois grupos: um com suplementação alimentar 30 dias antes do parto e outro sem suplementação. Os animais (ovelha e cordeiros foram subdivididos de acordo com a idade à desmama (45 ou 60 dias de idade e os cordeiros desmamados foram submetidos a três sistemas de terminação: confinamento com dieta completa; confinamento somente com feno; e confinamento somente no pasto. O abate dos cordeiros foi realizado aos 30 kg de peso vivo ou aos 150 dias de idade. As características de carcaça analisadas foram morfofisiologia da fibra do músculo longissimus dorsi, fragmentação miofibrilar pós-morte (maturados nos dias 0, 3 e 7 pos mortem e redução do pH e da temperatura da carne pós-abate. Não houve efeito da suplementação às ovelhas ou da idade à desmama sobre nenhuma das características avaliadas. A composição em fibras de contração lenta e oxidativa, contração rápida e oxidativa ou contração rápida e glicolítica não foi alterada pelos fatores em estudo, mas a área transversal das fibras foi menor nos cordeiros terminados com feno, assim como os valores de pH, temperatura e as medidas dos fragmentos de miofibrila. Com o aumento do tempo de maturação de 0 para 3 e 7 dias post mortem, houve redução do comprimento dos fragmentos de miofibrilas. O sistema de terminação de cordeiros em confinamento somente com feno interfere mais intensamente na qualidade da carne que o sistema de terminação a pasto ou em confinamento com dieta completa.

  6. A Decade of Progress in Understanding the Eruptions of Classical Novae

    Science.gov (United States)

    Shara, M. M.

    2014-12-01

    During the 11 years since the 2002 Sitges Nova conference, over 700 refereed papers dealing with classical novae have been published. Rather than spend 2.3 seconds reviewing each one, I've tried to focus on the main themes that have captured the interests of most researchers. I've also used, as examples, the most influential and cited papers in each subfield, though a decade from now some of my choices may seem dated, provincial, or flat-out wrong. The key topics that I address include theory and simulations of nova explosions; the recurrent novae; observations of ejecta; symbiotic novae; connections between novae and type Ia supernovae; connections between classical and dwarf novae; extragalactic novae; the maximum magnitude - rate of decline relationship; and a set of challenges and unanswered questions that I hope we will have made much progress on by the time we reassemble around 2024.

  7. The geographic accessibility of pharmacies in Nova Scotia

    Science.gov (United States)

    Heard, Deborah; Fisher, Judith; Douillard, Jay; Muzika, Greg; Sketris, Ingrid S.

    2013-01-01

    Introduction: Geographic proximity is an important component of access to primary care and the pharmaceutical services of community pharmacies. Variations in access to primary care have been found between rural and urban areas in Canadian and international jurisdictions. We studied access to community pharmacies in the province of Nova Scotia. Methods: We used information on the locations of 297 community pharmacies operating in Nova Scotia in June 2011. Population estimates at the census block level and network analysis were used to study the number of Nova Scotia residents living within 800 m (walking) and 2 km and 5 km (driving) distances of a pharmacy. We then simulated the impact of pharmacy closures on geographic access in urban and rural areas. Results: We found that 40.3% of Nova Scotia residents lived within walking distance of a pharmacy; 62.6% and 78.8% lived within 2 km and 5 km, respectively. Differences between urban and rural areas were pronounced: 99.2% of urban residents lived within 5 km of a pharmacy compared with 53.3% of rural residents. Simulated pharmacy closures had a greater impact on geographic access to community pharmacies in rural areas than urban areas. Conclusion: The majority of Nova Scotia residents lived within walking or short driving distance of at least 1 community pharmacy. While overall geographic access appears to be lower than in the province of Ontario, the difference appears to be largely driven by the higher proportion of rural dwellers in Nova Scotia. Further studies should examine how geographic proximity to pharmacies influences patients’ access to traditional and specialized pharmacy services, as well as health outcomes and adherence to therapy. Can Pharm J 2013;146:39-46. PMID:23795168

  8. X-ray Observations of Novae with Swift

    Science.gov (United States)

    Page, Kim

    2016-07-01

    The rapid response capabilities of the Swift satellite, together with the daily planning of its observing schedule, make it an ideal mission for following novae in the X-ray and UV bands, particularly during their early phases of rapid evolution. A number of both classical and recurrent novae have been extensively monitored by Swift throughout their super-soft phase and later decline. We report results from these observations, including the high-amplitude flux variation often see at the start of the super-soft emission, the differing relationships between the X-ray and UV variability, and the spectral evolution seen in the X-ray band.

  9. V445 Puppis, a first identified helium nova

    Directory of Open Access Journals (Sweden)

    Mariko Kato

    2004-01-01

    Full Text Available La explosi on de 2001 de V445 Puppis ha mostrado que se trata de un objeto unico que presenta ausencia de hidr ogeno, enriquecimiento de helio y carbono y una lenta ca da de la curva de luz con una amplitud peque~na. Hemos calculado curvas de luz te oricas de novas de helio para con rmar que V445 Pup es el primer ejemplo de una nova de helio. Del ajuste de la curva de luz podemos concluir que la enana blanca es muy masiva 1:33M .

  10. Nova in Ophiuchus - TCP J17394608-2457555

    Science.gov (United States)

    Waagen, Elizabeth O.

    2017-05-01

    AAVSO Alert Notice 576 announces the discovery of a galactic nova in Ophiuchus, TCP J17394608-2457555, by Koichi Itagaki (Yamagata, Japan) at unfiltered CCD magnitude 13.6 on 2017 May 08.7511 UT. Spectroscopy indicating that TCP J17394608-2457555 is an FeII nova (highly reddened) was obtained 2017 May 11.15 UT by S. C. Wiliams (Lancaster) and M. J. Darnley (LJMU) (ATel #10366). Finder charts with sequence may be created using the AAVSO Variable Star Plotter (https://www.aavso.org/vsp). Observations should be submitted to the AAVSO International Database. See full Alert Notice for more details.

  11. Liquid scintillator production for the NOvA experiment

    Energy Technology Data Exchange (ETDEWEB)

    Mufson, S., E-mail: mufson@indiana.edu [Indiana University, Bloomington, IN 47405 (United States); Baugh, B.; Bower, C. [Indiana University, Bloomington, IN 47405 (United States); Coan, T.E. [Southern Methodist University, Dallas, TX 75275 (United States); Cooper, J. [Fermi National Accelerator Laboratory, Batavia, IL 60510 (United States); Corwin, L. [South Dakota School of Mines and Technology, Rapid City, SD 57701 (United States); Karty, J.A. [Indiana University, Bloomington, IN 47405 (United States); Mason, P. [University of Tennessee, Knoxville, TN 37916 (United States); Messier, M.D. [Indiana University, Bloomington, IN 47405 (United States); Pla-Dalmau, A. [Fermi National Accelerator Laboratory, Batavia, IL 60510 (United States); Proudfoot, M. [Renkert Oil, Morgantown, PA 19543 (United States)

    2015-11-01

    The NOvA collaboration blended and delivered 8.8 kt (2.72M gal) of liquid scintillator as the active detector medium to its near and far detectors. The composition of this scintillator was specifically developed to satisfy NOvA's performance requirements. A rigorous set of quality control procedures was put in place to verify that the incoming components and the blended scintillator met these requirements. The scintillator was blended commercially in Hammond, IN. The scintillator was shipped to the NOvA detectors using dedicated stainless steel tanker trailers cleaned to food grade.

  12. The unreasonable effectiveness of experiments in constraining nova nucleosynthesis

    Directory of Open Access Journals (Sweden)

    Parikh Anuj

    2014-01-01

    Full Text Available Classical nova explosions arise from thermonuclear ignition in the envelopes of accreting white dwarfs in close binary star systems. Detailed observations of novae have stimulated numerous studies in theoretical astrophysics and experimental nuclear physics. These phenomena are unusual in nuclear astrophysics because most of the thermonuclear reaction rates thought to be involved are constrained by experimental measurements. This situation allows for rather precise statements to be made about which measurements are still necessary to improve the nuclear physics input to astrophysical models. We briefly discuss desired measurements in these environments with an emphasis on recent experimental progress made to better determine key rates.

  13. NovaNET User Manual for C-Router Instructors. Second Edition Revised.

    Science.gov (United States)

    Fortner, Monica B.; Davis, Dennis M.

    The NovaNET computer system is a mainframe system with a large network of users sharing the same computer. This manual is intended to teach instructors how to use the NovaNET system to deliver instruction to their students. The manual is divided into four main sections, each of which teaches a group of skills needed by NovaNET instructors. The…

  14. NovaNET User Manual for C-Router Instructors. Second Edition Revised.

    Science.gov (United States)

    Fortner, Monica B.; Davis, Dennis M.

    The NovaNET computer system is a mainframe system with a large network of users sharing the same computer. This manual is intended to teach instructors how to use the NovaNET system to deliver instruction to their students. The manual is divided into four main sections, each of which teaches a group of skills needed by NovaNET instructors. The…

  15. Swift X-Ray Observations of Classical Novae. II. The Super Soft Source sample

    CERN Document Server

    Schwarz, Greg J; Osborne, J P; Page, K L; Evans, P A; Beardmore, A P; Walter, Frederick M; Helton, L Andrew; Woodward, Charles E; Bode, Mike; Starrfield, Sumner; Drake, Jeremy J

    2011-01-01

    The Swift GRB satellite is an excellent facility for studying novae. Its rapid response time and sensitive X-ray detector provides an unparalleled opportunity to investigate the previously poorly sampled evolution of novae in the X-ray regime. This paper presents Swift observations of 52 Galactic/Magellanic Cloud novae. We included the XRT (0.3-10 keV) X-ray instrument count rates and the UVOT (1700-8000 Angstroms) filter photometry. Also included in the analysis are the publicly available pointed observations of 10 additional novae the X-ray archives. This is the largest X-ray sample of Galactic/Magellanic Cloud novae yet assembled and consists of 26 novae with super soft X-ray emission, 19 from Swift observations. The data set shows that the faster novae have an early hard X-ray phase that is usually missing in slower novae. The Super Soft X-ray phase occurs earlier and does not last as long in fast novae compared to slower novae. All the Swift novae with sufficient observations show that novae are highly v...

  16. The Wendelstein Calar Alto Pixellensing Project (WeCAPP): the M 31 nova catalogue

    Science.gov (United States)

    Lee, C.-H.; Riffeser, A.; Seitz, S.; Bender, R.; Fliri, J.; Hopp, U.; Ries, C.; Bärnbantner, O.; Gössl, C.

    2012-01-01

    We present light curves from the novae detected in the long-term, M 31-monitoring WeCAPP project. The goal of WeCAPP is to constrain the compact dark matter fraction of the M 31 halo with microlensing observations. As a by product we detected 91 novae benefiting from the high cadence and highly sensitive difference imaging technique required for pixel-lensing. We thus can now present the largest sample of optical/CCD nova lightcurves towards M 31 to date. We also obtained thorough coverage of the light curve before and after the eruption thanks to the long-term monitoring. We apply a nova taxonomy to our nova candidates and found 29 S-class novae, 10 C-class novae, 2 O-class novae, and 1 J-class nova. We investigated a universal decline law on the S-class novae. In addition, we correlated our catalogue with the literature and found 4 potential recurrent novae. Part of our catalogue has been used to search for optical counterparts of the super soft X-ray sources detected in M 31. Optical surveys like WeCAPP, when coordinated with multi-wavelength observation, will continue to shed light on the underlying physical mechanism of novae in the future.

  17. Dique seco de carena. Génova

    Directory of Open Access Journals (Sweden)

    Gai, Luigi

    1965-02-01

    Full Text Available After elaborate planning, the building, towing and sinking of the ship repairing dry dock at Genoa has now been completed. The dock is 260x52x21.5 m in size. Its structure is cellular and it is made of reinforced and prestressed concrete. A special feature of this dock is that it rests on a flexible bed of sand, dredged from the sea bed. To prepare this, the following operations were carried out: mud was first dredged away, the stony outcrops were levelled off, the spaces in between the rocks were filled with concrete, then the layer of sand was placed, and finally a surface of larger aggregate was prepared on top. The method of attaching the dock to the sea bed to ensure its stability is also noteworthy. After much thought, it was decided that once the dock was sunk at its final emplacement, if its cellular compartments were filled with sand ballast, its own weight would ensure its permanent stability in the face of rough seas. The maneuvers for floating the dock, and sinking it, were also complex, since it was essential to take carefully into account the state of the weather. Any storm might have severely damaged the dock's cellular structure. The prefabrication of the caissons, the jointing of them into a large structure, the construction of enclosing walls, the provision of galleries, companionways, and housing facilities inside the dock, and the towing, sinking and ballasting of this large and heavy structure, constitute a series of building and navigational operations of great complexity, which have tested the ability of the firm Fincosit, who specialise in hydraulic projects.Después de profundos estudios se ha terminado recientemente la construcción, remolque y hundimiento del dique seco de carena del puerto de Génova, cuyas dimensiones son: 260x52x21,5 metros. Es de estructura celular, y de hormigón armado y pretensado. La particularidad de la obra estriba en el apoyo de la plataforma sobre un lecho flexible de arena dragada del mar

  18. Development of the Hα profile in Nova Del 2013

    Science.gov (United States)

    Storrs, Alex; Mahmoudian, T.

    2014-01-01

    We report observations of the Hα profile of Nova Del 2013, with resolving power R = 3000. Starting in late August the expected P Cygni profile (blueshifted absorption) was observed. Beginning in September a redshifted absorption appears and strengthens through the month. We will report observations through fall and discuss possible causes of these features.

  19. 3D Hydrodynamic Simulation of Classical Novae Explosions

    Science.gov (United States)

    Kendrick, Coleman J.

    2015-01-01

    This project investigates the formation and lifecycle of classical novae and determines how parameters such as: white dwarf mass, star mass and separation affect the evolution of the rotating binary system. These parameters affect the accretion rate, frequency of the nova explosions and light curves. Each particle in the simulation represents a volume of hydrogen gas and are initialized randomly in the outer shell of the companion star. The forces on each particle include: gravity, centrifugal, coriolis, friction, and Langevin. The friction and Langevin forces are used to model the viscosity and internal pressure of the gas. A velocity Verlet method with a one second time step is used to compute velocities and positions of the particles. A new particle recycling method was developed which was critical for computing an accurate and stable accretion rate and keeping the particle count reasonable. I used C++ and OpenCL to create my simulations and ran them on two Nvidia GTX580s. My simulations used up to 1 million particles and required up to 10 hours to complete. My simulation results for novae U Scorpii and DD Circinus are consistent with professional hydrodynamic simulations and observed experimental data (light curves and outburst frequencies). When the white dwarf mass is increased, the time between explosions decreases dramatically. My model was used to make the first prediction for the next outburst of nova DD Circinus. My simulations also show that the companion star blocks the expanding gas shell leading to an asymmetrical expanding shell.

  20. Sorveglianza sistematica dell'ex-nova GK Persei.

    Science.gov (United States)

    Dalmeri, I.; Favero, G.; Milani, G. A.; Tonello, A.; Monella, R.

    The 1983 and 1986 optical outbursts of the old-nova GK Per (1901) obeyed to the rule of quasi-periodicity proposed by Sabbadin and Bianchini. During the outbursts the colour indexes (U-B), (B-V) and (V-R) showed a behaviour opposite to the luminosity of the star.

  1. Optical spectroscopy of the dwarf nova U Geminorum

    NARCIS (Netherlands)

    Unda-Sanzana, E.; Marsh, T.R.; Morales-Rueda, L.

    2006-01-01

    The dwarf nova U Gem is unique in having a direct measurement of the K velocity of its white dwarf from Hubble Space Telescope (HST) spectra (K1 = 107 +/- 2kms-1 from Long et al.). We present high-resolution optical spectra of U Gem in quiescence taken to test the accuracy to w

  2. The Formation of Cataclysmic Variables: The Influence of Nova Eruptions

    Science.gov (United States)

    Nelemans, G.; Siess, L.; Repetto, S.; Toonen, S.; Phinney, E. S.

    2016-01-01

    The theoretical and observed populations of pre-cataclysmic variables are dominated by systems with low-mass white dwarfs (WDs), while the WD masses in cataclysmic variables (CVs) are typically high. In addition, the space density of CVs is found to be significantly lower than in the theoretical models. We investigate the influence of nova outbursts on the formation and initial evolution of CVs. In particular, we calculate the stability of the mass transfer in the case where all of the material accreted on the WD is lost in classical novae and part of the energy to eject the material comes from a common-envelope-like interaction with the companion. In addition, we study the effect of an asymmetry in the mass ejection that may lead to small eccentricities in the orbit. We find that a common-envelope-like ejection significantly decreases the stability of the mass transfer, particularly for low-mass WDs. Similarly, the influence of asymmetric mass loss can be important for short-period systems and even more so for low-mass WDs; however, this influence likely disappears long before the next nova outburst due to orbital circularization. In both cases the mass-transfer rates increase, which may lead to observable (and perhaps already observed) consequences for systems that do survive to become CVs. However, a more detailed investigation of the interaction between nova ejecta and the companion and the evolution of slightly eccentric CVs is needed before definite conclusions can be drawn.

  3. Parasites of red foxes in New Brunswick and Nova Scotia.

    Science.gov (United States)

    Smith, H J

    1978-07-01

    Sixty-one red foxes from New Brunswick and Nova Scotia were examined for helminths. Alaria americana, A. arisaemoides, A. mustelae, Cryptocotyle lingua, Echinostoma revolution and Metorchis conjunctus, Capillaria aerophila, Crenosoma vulpis, Toxocara canis, Uncinaria stenocephala and Taenia crassiceps were found. Approximately 67% of the foxes examined were clinically affected with Sarcoptes scabiei mange.

  4. The awakening of a classical nova from hibernation

    CERN Document Server

    Mroz, P; Pietrukowicz, P; Szymanski, M K; Soszynski, I; Wyrzykowski, L; Poleski, R; Kozlowski, S; Skowron, J; Ulaczyk, K; Skowron, D; Pawlak, M

    2016-01-01

    Cataclysmic variable stars (CVs) are close binary systems consisting of a white dwarf (primary) that is accreting matter from a low-mass companion star (secondary). From time to time such systems undergo large-amplitude brightenings. The most spectacular eruptions, over $10^4$ times in brightness, occur in classical novae and are caused by a thermonuclear runaway on the surface of the white dwarf. Such eruptions are thought to recur on timescales of $10^4-10^6$. In between, the system's properties depend primarily on the mass-transfer rate: if it is lower than a $10^{-9} M_{\\odot}$/year, the accretion becomes unstable and the matter is dumped onto the white dwarf during quasi-periodic dwarf nova outbursts. The hibernation hypothesis predicts that nova eruptions strongly affect the mass-transfer rate, keeping it high for centuries after the event. Subsequently, the mass-transfer rate should significantly decrease for $10^3-10^6$ years, starting the hibernation phase. After that the nova awakes again - with acc...

  5. Luminous Red Nova 2015 in the Galaxy M101

    CERN Document Server

    Goranskij, V P; Spiridonova, O I; Valeev, A F; Fatkhullin, T A; Moskvitin, A S; Vozyakova, O V; Cheryasov, D V; Safonov, B S; Zharova, A V; Hancock, T

    2016-01-01

    We present the results of the study of the red nova PSN J14021678+5426205 based on the observations carried out with the Russian 6-m telescope (BTA) along with other telescopes of SAO RAS and SAI MSU. To investigate the nova progenitor, we used the data from the Digital Sky Survey and amateur photos available on the internet. In the period between April 1993 and July 2014, the brightness of the progenitor gradually increased by 2.2 mag in the V band. At the peak of the first outburst in mid-November of 2014, the star reached an absolute visual magnitude of -12.75 mag but was discovered later, in February 2015, in a repeated outburst at the absolute magnitude of -11.65 mag. The amplitude of the outburst was minimum among the red novae, only 5.6 mag in the V band. The H alpha emission line and the continuum of a cool supergiant with a gradually decreasing surface temperature were observed in the spectra. Such process is typical for red novae, although the object under study showed extreme parameters: maximum lu...

  6. A Dwarf Nova in the Globular Cluster M13

    NARCIS (Netherlands)

    Servillat, M.; Webb, N.A.; Lewis, F.; Knigge, C.; van den Berg, M.C.; Dieball, A.; Grindlay, J.E.

    2011-01-01

    Dwarf novae (DNe) in globular clusters (GCs) seem to be rare with only 13 detections in the 157 known Galactic GCs. We report the identification of a new DN in M13, the 14th DN identified in a GC to date. Using the 2 m Faulkes Telescope North, we conducted a search for stars in M13 that show variabi

  7. Parnassiana nova : XVII. Kritische Revision der Gattung Parnassius (Fortsetzung 12)

    NARCIS (Netherlands)

    Eisner, C.

    1957-01-01

    Meine in Parnassiana Nova VIII wiedergegebene Beurteilung der spanischen apollo-subspecies muss ich aufgrund der grossen Serien davon, die ich aus Sammlung R. Oberthür erworben habe, und aufgrund des Gedankenaustausches mit Dr. W. Marten teilweise berichtigen. subsp. chrysophorus Fruhst., die

  8. TV review: Nova scienceNOW - Season 2, Episode 4

    CERN Document Server

    Lasser, Josh

    2007-01-01

    "Sitting down to watch the fourth episode of the second season of Nova ScienceNOW I'm mainly struck by one thought: why have they only put out four epidoses nearly nine months into their second season? The second story is all about CERN and the LHC. (2 pages)

  9. Parnassiana nova : XVII. Kritische Revision der Gattung Parnassius (Fortsetzung 12)

    NARCIS (Netherlands)

    Eisner, C.

    1957-01-01

    Meine in Parnassiana Nova VIII wiedergegebene Beurteilung der spanischen apollo-subspecies muss ich aufgrund der grossen Serien davon, die ich aus Sammlung R. Oberthür erworben habe, und aufgrund des Gedankenaustausches mit Dr. W. Marten teilweise berichtigen. subsp. chrysophorus Fruhst., die niedri

  10. Discovery of a Probable Nova in M81

    Science.gov (United States)

    Hornoch, K.; Vaduvescu, O.; Mocnik, T.

    2014-09-01

    We report the discovery of a probable nova in M81 on a co-added 1440-s narrow-band H-alpha CCD image taken with the 2.5-m Isaac Newton Telescope (INT) + WFC at La Palma under ~2.2" seeing on 2014 Sep.

  11. Hydrodynamic studies of oxygen, neon, and magnesium novae

    Science.gov (United States)

    Starrfield, Sumner; Sparks, W. M.; Truran, J. W.

    1987-01-01

    Results are presented from recent theoretical studies that have examined the properties of nova outbursts on ONeMg white dwarfs. These outbursts are much more violent and occur much more frequently than outbursts on CO white dwarfs. Hydrodynamic simulations of both kinds of outbursts are in excellent agreement with the observations.

  12. The Present Status of the Antigonish Movement in Nova Scotia.

    Science.gov (United States)

    Sowder, Ellie Mae

    A comprehensive case study is presented of the Antigonish Movement in eastern Nova Scotia. Originally founded to combat poverty and exploitation, it has functioned since 1929 under the extension department of St. Francis Xavier University, Antigonish. The Movement brought education into the lives of ordinary working people and introduced group…

  13. The Nova Upgrade Facility for ICF ignition and gain

    Science.gov (United States)

    Lowdermilk, W. H.; Campbell, E. M.; Hunt, J. T.; Murray, J. R.; Storm, E.; Tobin, M. T.; Trenholme, J. B.

    1992-01-01

    Research on Inertial Confinement Fusion (ICF) is motivated by its potential defense and civilian applications, including ultimately the generation of electric power. The U.S. ICF Program was reviewed recently by the National Academy of Science (NAS) and the Fusion Policy Advisory Committee (FPAC). Both committees issued final reports in 1991 which recommended that first priority in the ICF program be placed on demonstrating fusion ignition and modest gain (G less than 10). The U.S. Department of Energy and Lawrence Livermore National Laboratory (LLNL) have proposed an upgrade of the existing Nova Laser Facility at LLNL to accomplish these goals. Both the NAS and FPAC have endorsed the upgrade of Nova as the optimal path to achieving ignition and gain. Results from Nova Upgrade Experiments will be used to define requirements for driver and target technology both for future high-yield military applications, such as the Laboratory Microfusion Facility (LMF) proposed by the Department of Energy, and for high-gain energy applications leading to an ICF engineering test facility. The central role and modifications which Nova Upgrade would play in the national ICF strategy are described.

  14. Radiative shocks create environments for dust formation in classical novae

    Science.gov (United States)

    Derdzinski, Andrea M.; Metzger, Brian D.; Lazzati, Davide

    2017-08-01

    Classical novae commonly show evidence of rapid dust formation within months of the outburst. However, it is unclear how molecules and grains are able to condense within the ejecta, given the potentially harsh environment created by ionizing radiation from the white dwarf. Motivated by the evidence for powerful radiative shocks within nova outflows, we propose that dust formation occurs within the cool, dense shell behind these shocks. We incorporate a simple molecular chemistry network and classical nucleation theory with a model for the thermodynamic evolution of the post-shock gas, in order to demonstrate the formation of both carbon and forsterite (Mg2SiO4) grains. The high densities due to radiative shock compression (n ∼ 1014 cm-3) result in CO saturation and rapid dust nucleation. Grains grow efficiently to large sizes ≳ 0.1 μm, in agreement with IR observations of dust-producing novae, and with total dust masses sufficient to explain massive extinction events such as V705 Cas. As in dense stellar winds, dust formation is CO-regulated, with carbon-rich flows producing carbon-rich grains and oxygen-rich flows primarily forming silicates. CO is destroyed by non-thermal particles accelerated at the shock, allowing additional grain formation at late times, but the efficiency of this process appears to be low. Given observations showing that individual novae produce both carbonaceous and silicate grains, we concur with previous works attributing this bimodality to chemical heterogeneity of the ejecta. Nova outflows are diverse and inhomogeneous, and the observed variety of dust formation events can be reconciled by different abundances, the range of shock properties, and the observer viewing angle. The latter may govern the magnitude of extinction, with the deepest extinction events occurring for observers within the binary equatorial plane.

  15. Are presolar dust grains from novae actually from supernovae?

    Science.gov (United States)

    Nittler, L. R.; Hoppe, P.

    2005-05-01

    Meteorites contain presolar stardust grains that formed in prior generations of stars and exhibit large isotopic anomalies reflecting the nuclear processes that occurred in their individual parent stars. RGB and AGB stars and supernovae are well established as sources of many of these grains. Novae have been proposed as sources for a few SiC and graphite grains with low 12}C/{13C and 14}N/{15N ratios and unusual Si isotopic ratios (Amari et al., ApJ, 551, 1065). We have found three SiC grains from the Murchison meteorite with C and N isotopic ratios similar to the previously-reported putative nova grains. However, the isotopic signatures of Si, Ca, Al and Ti in one of the grains (334-2) clearly indicate a supernova origin, especially excess 28Si correlated with excess 44Ca. The latter signature is attributable to in situ decay of (half-life=50yr) 44Ti. Another 13C- and 15N-rich grain (151-4) has a large 47Ti enrichment. This signature is not expected for nova nucleosynthesis. Thus, the new isotopic data raise the possibility that the grains previously reported to have formed in novae actually formed in supernovae, and that novae have not left a record in the presolar grain populations that have been so far studied. Moreover, the results in grain 334-2 indicate that supernovae contain regions highly enriched in both 13C and 15N. This is not predicted by current models but may bear on the cosmic origin of 15N. This work was funded in part by NASA.

  16. The Wendelstein Calar Alto Pixellensing Project (WeCAPP): the M31 Nova catalogue

    CERN Document Server

    Lee, C -H; Seitz, S; Bender, R; Fliri, J; Hopp, U; Ries, C; Baernbantner, O; Goessl, C

    2011-01-01

    We present light curves from the novae detected in the long-term, M31 monitoring WeCAPP project. The goal of WeCAPP is to constrain the compact dark matter fraction of the M31 halo with microlensing observations. As a by product we have detected 91 novae benefiting from the high cadence and highly sensitive difference imaging technique required for pixellensing. We thus can now present the largest CCD and optical filters based nova light curve sample up-to-date towards M31. We also obtained thorough coverage of the light curve before and after the eruption thanks to the long-term monitoring. We apply the nova taxonomy proposed by Strope et al. (2010) to our nova candidates and found 29 S-class novae, 10 C-class novae, 2 O-class novae and 1 J-class nova. We have investigated the universal decline law advocated by Hachichu and Kato (2006) on the S-class novae. In addition, we correlated our catalogue with the literature and found 4 potential recurrent novae. Part of our catalogue has been used to search for opt...

  17. The UBV Color Evolution of Classical Novae. II. Color-Magnitude Diagram

    CERN Document Server

    Hachisu, Izumi

    2016-01-01

    We have examined the outburst tracks of 40 novae in the color-magnitude diagram (intrinsic B-V color versus absolute V magnitude). After reaching the optical maximum, each nova generally evolves toward blue from the upper-right to the lower-left and then turns back toward the right. The 40 tracks are categorized into one of six templates: very fast nova V1500 Cyg; fast novae V1668 Cyg, V1974 Cyg, and LV Vul; moderately fast nova FH Ser; and very slow nova PU Vul. These templates are located from the left (blue) to the right (red) in this order, depending on the envelope mass and nova speed class. A bluer nova has a less massive envelope and faster nova speed class. In novae with multiple peaks, the track of the first decay is more red than that of the second (or third) decay, because a large part of the envelope mass had already been ejected during the first peak. Thus, our newly obtained tracks in the color-magnitude diagram provide useful information to understand the physics of classical novae. We also fou...

  18. Tallinna Ülikooli Balti Filmi- ja Meediakooli õppehoone Nova = Tallinn University Baltic Film and Media School "Nova"

    Index Scriptorium Estoniae

    2015-01-01

    Tallinna Ülikooli Balti Filmi- ja Meediakooli õppehoone "Nova" Narva maantee 27, valminud 2012. Arhitektuuri sihtkapitali arhitektuuripreemia 2012 ja Arhitektuuri sihtkapitali sisearhitektuuripreemia 2013. Arhitektid Maarja Kask, Karli Luik, Ralf Lõoke, Pelle-Sten Viiburg (Salto Arhitektid). Sisearhitektid Ville Lausmäe, Kadi Karmann (VLS). Mööbel Ville Lausmäe, Tõnis Kalve. Konstruktor Jaanus Natka (EA Reng)

  19. Tallinna Ülikooli Balti Filmi- ja Meediakooli õppehoone Nova = Tallinn University Baltic Film and Media School "Nova"

    Index Scriptorium Estoniae

    2015-01-01

    Tallinna Ülikooli Balti Filmi- ja Meediakooli õppehoone "Nova" Narva maantee 27, valminud 2012. Arhitektuuri sihtkapitali arhitektuuripreemia 2012 ja Arhitektuuri sihtkapitali sisearhitektuuripreemia 2013. Arhitektid Maarja Kask, Karli Luik, Ralf Lõoke, Pelle-Sten Viiburg (Salto Arhitektid). Sisearhitektid Ville Lausmäe, Kadi Karmann (VLS). Mööbel Ville Lausmäe, Tõnis Kalve. Konstruktor Jaanus Natka (EA Reng)

  20. Composição corporal e exigências nutricionais de energia e proteína para cordeiros em crescimento Corporal composition and nutritional requirements for energy and protein of growing lambs

    Directory of Open Access Journals (Sweden)

    Cleber Cassol Pires

    2000-06-01

    Full Text Available Este trabalho foi realizado com o objetivo de determinar a composição corporal para gordura, proteína e cinzas, as exigências líquidas de energia e proteína para ganho de peso e as exigências de proteína metabolizável de cordeiros em crescimento. Foram utilizados 22 cordeiros machos inteiros, filhos de carneiros Texel e ovelhas cruzas (Texel x Ideal; destes, quatro foram abatidos no início do experimento (24 horas após o nascimento e grupos de seis cordeiros, ao desmame, aos 28 e 33 kg de peso vivo. As equações de predição da composição corporal de proteína, gordura, cinzas e energia foram realizadas de acordo com o ARC (1980, por intermédio da regressão do logaritmo de proteína, gordura, cinzas e energia no corpo vazio, em relação ao logaritmo do peso de corpo vazio (PCV. As exigências líquidas de proteína e energia para ganho de peso foram obtidas por meio das equações de predição da composição corporal, ao passo que as exigências de proteína metabolizável foram estimadas de acordo com o AFRC (1993. Os conteúdos corporais de proteína, gordura, energia e matéria mineral para cordeiros de 5 a 30 kg PCV variaram de 141,69 a 186,24 g/kg PCV; 24,49 a 158,11 g/kg PCV; 1088,75 a 2451,55 kcal/kg PCV; e 27,55 a 33,70 g/kg PCV, respectivamente. As estimativas das exigências líquidas para ganho foram: energia, 399,93 e 892,21 kcal/250g de ganho, e proteína de 40,98 e 53,70 g/250g de ganho, para cordeiros de 5 e 30 kg de PCV, respectivamente. As exigências de proteína metabolizável para animais de 5 e 30 kg de peso vivo foram de 79,09 a 121,13 g/250g de ganho.This work was conducted with the objective to determine the body composition for fat, protein and ash, the net requirements of energy and protein for weight gain, and the requirements of metabolizable protein of growing lambs. Twenty-two male lambs, sired by Texel males, from crossbreed Texel x Ideal dams were used. Four lambs were slaughtered at the

  1. Classical novae from the POINT-AGAPE microlensing survey of M31 -- I. The nova catalogue

    CERN Document Server

    Darnley, Matt J.; Kerins, E.; Newsam, A.M.; An, J.; Baillon, P.; Calchi Novati, S.; Carr, Bernard J.; Creze, M.; Evans, N.W.; Giraud-Heraud, Y.; Gould, A.; Hewett, Paul C.; Jetzer, Ph.; Kaplan, J.; Paulin-Henriksson, S.; Smartt, S.J.; Stalin, C.S.; Tsapras, Y.

    2004-01-01

    The POINT-AGAPE survey is an optical search for gravitational microlensing events towards the Andromeda Galaxy (M31). As well as microlensing, the survey is sensitive to many different classes of variable stars and transients. Here we describe the automated detection and selection pipeline used to identify M31 classical novae (CNe) and we present the resulting catalogue of 20 CN candidates observed over three seasons. CNe are observed both in the bulge region as well as over a wide area of the M31 disk. Nine of the CNe are caught during the final rise phase and all are well sampled in at least two colours. The excellent light-curve coverage has allowed us to detect and classify CNe over a wide range of speed class, from very fast to very slow. Among the light-curves is a moderately fast CN exhibiting entry into a deep transition minimum, followed by its final decline. We have also observed in detail a very slow CN which faded by only 0.01 mag day$^{-1}$ over a 150 day period. We detect other interesting varia...

  2. Fresh and matured lamb meat quality fed with sunflower seeds and vitamin E Qualidade da carne in natura e maturada de cordeiros alimentados com grãos de girassol e vitamina E

    Directory of Open Access Journals (Sweden)

    Ronaldo Oliveira Sales

    2013-01-01

    Full Text Available The objective of the study is to evaluate meat quality from Ile de France lamb fed diets supplemented with sunflower seeds and vitamin E. Thirty-two lamb weighing initially 15kg were housed in individual stalls and slaughtered when body weight reached 32kg. The treatments consisted of four experimental diets: D1 sugarcane + concentrate without sunflower seeds; D2 sugarcane + concentrate with sunflower seeds; D3 sugarcane + concentrate without sunflower seeds plus 1000mg vitamin E kg-1 diet dry matter (DM; and D4 sugarcane + concentrate with sunflower seeds and 1000mg vitamin E kg-1 diet DM. The parameters temperature, pH, color, cooking loss, shear force and water holding capacity were determined at maturation times of 0, 7 and 14 days on the Longissimus dorsi muscle. Qualitative characteristics of the meat were not affected by the sunflower seed combined with vitamin E diet; however, pH 24 hours was affected (P0.05 by diet or maturation times. On the other hand, shear force and water holding capacity were significantly affected (PO objetivo deste estudo foi avaliar a qualidade da carne de cordeiros Ile de France alimentados com dietas contendo grãos de girassol e vitamina E. Trinta e dois cordeiros pesando inicialmente 15kg foram alojados em baias individuais e abatidos ao atingir 32kg de peso corporal. Os tratamentos consistiram de quatro dietas experimentais: D1 cana-de-açúcar + concentrado sem grãos de girassol; D2 cana-de-açúcar + concentrado com grãos de girassol; D3 cana-de-açúcar + concentrado grãos de girassol, mais 1000mg de vitamina E kg-1 de matéria seca (MS da dieta; e D4 cana-de-açúcar + concentrado com grãos de girassol e 1000mg de vitamina E dieta kg-1 de MS. Os parâmetros temperatura, pH, cor, perda de peso ao cozimento, força de cisalhamento e capacidade de retenção de água foram determinados nos tempos de maturação de 0, 7 e 14 dias no músculo Longissimus dorsi. As características qualitativas da carne n

  3. Características da carcaça de cordeiros alimentados com dietas contendo diferentes níveis de fibra em detergente neutro Carcass characteristics of lambs fed diets with different neutral detergent fiber levels

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    Cleber Cassol Pires

    2006-10-01

    Full Text Available Este estudo foi conduzido com o objetivo de avaliar o efeito de diferentes níveis de FDN na dieta sobre as características de carcaça de cordeiros confinados e abatidos com 30 kg de PV. Foram utilizados 20 cordeiros machos, não-castrados, cruza Ile de France x Texel, distribuídos aleatoriamente em quatro tratamentos (25, 31, 37 e 43% de FDN na dieta. O volumoso utilizado foi silagem de sorgo híbrido (AG 2005 E e o concentrado foi composto de milho desintegrado, farelo de soja, sal comum, calcário calcítico e fosfato bicálcico. As dietas foram isoprotéicas (17% de PB e as características avaliadas foram: peso de carcaça quente (PCQ, peso de carcaça fria (PCF, rendimento de carcaça quente (RCQ, rendimento de carcaça fria (RCF, índice de quebra ao resfriamento (IQ, área de olho-de-lombo (AOL, espessura de gordura subcutânea (EG, comprimento da carcaça (CC, largura da perna (LP, profundidade do peito (PPEITO, comprimento de perna (CPERNA, peso e proporção de perna, paleta, costilhar e pescoço e pesos e proporções de osso, músculo e gordura da perna dos cordeiros. O aumento do nível de FDN nas dietas reduziu linearmente o PCQ, PCF, RCQ, RCF e o peso de costilhar. Houve efeito quadrático do nível de FDN sobre o CPERNA. As demais variáveis analisadas não foram influenciadas pelos níveis de FDN das dietas.The objective of this trial was to evaluate the effect of different dietary NDF levels on carcass characteristics of feedlot lambs slaughtered with 30 kg of body weight. Twenty crossbred Ile de France x Texel non-castrated male lambs were randomly assigned to the following treatments: 25%, 31%, 37%, and 43% of dietary NDF. The forage portion of the diet was composed by sorghum silage (hybrid AG 2005 E and the concentrate by cracked corn, soybean meal, salt, limestone, and dicalcium phosphate. Diets were isonitrogenous averaging 17% of crude protein. The following variables were measured: hot carcass weight (HCW, cold

  4. Qualidade da carne de cordeiros criados em creep feeding com silagem de grãos úmidos de milho Meat quality of lambs fed with high moisture corn silage in creep feeding

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    Gercílio Alves de Almeida Júnior

    2004-08-01

    Full Text Available Objetivou-se, com este trabalho, estudar níveis de substituição (0; 50 e 100% do milho grão seco moído pela silagem de grãos úmidos de milho (SGUM na ração de cordeiros alimentados em creep feeding. Vinte e quatro cordeiros Suffolk foram avaliados quanto às características quantitativas e qualitativas do músculo longissimus dorsi. Os animais foram abatidos ao atingirem 28 kg PV e suas carcaças resfriadas foram seccionadas em sete regiões anatômicas. Sobre a superfície do longissimus dorsi, no corte denominado lombo, foram tomadas as medidas: largura e profundidade máximas; mínima e máxima espessuras de gordura de cobertura e área de olho de lombo. Nos lombos, determinaram-se as proporções dos tecidos muscular, adiposo e ósseo, a composição química e a força de cisalhamento. Os resultados revelaram que não houve efeito dos tratamentos para a força de cisalhamento e nem para as medidas tomadas no longissimus dorsi, exceto para a área de olho de lombo, segundo regressão quadrática, com maiores valores para os tratamentos com SGUM. As análises de composição química do longissimus dorsi revelaram que os tratamentos influenciaram o teor de gordura no músculo, que aumentou linearmente de acordo com a inclusão de SGUM na ração. Não foi verificado efeito dos tratamentos sobre a composição tecidual dos lombos. Concluiu-se que é possível recomendar a substituição do milho grão pela silagem de grãos úmidos de milho para a dieta de cordeiros terminados em creep feeding, conservando a boa qualidade da carne.The experiment was carried to study three three levels (0, 50 e 100% of high moisture corn silage replacing dry corn grain in rations of lambs fed in creep feeding. Twenty four Suffolk lambs were evaluated to qualitative and quantitative loin (longissimus dorsi characteristics. Lambs were weighed until to reach pre-fixed slaughter weight, 28 kg LW. Cold carcasses were cut in seven anatomical regions. Four

  5. Desempenho e características da carcaça de cordeiros confinados alimentados com grãos de soja Performance and carcass characteristics of feedlot lambs fed raw soybean

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    Fumi Shibata Urano

    2006-10-01

    Full Text Available O objetivo deste trabalho foi avaliar a influência de grãos de soja (GS no desempenho, características e rendimento de cortes de carcaça de cordeiros confinados. Sessenta e quatro cordeiros Santa Inês, com peso vivo inicial de 19,5±0,19 kg e 75±2 dias de idade, foram distribuídos em blocos ao acaso de acordo com o peso vivo e a idade no início do experimento. Os GS participaram com 0, 7, 14 e 21% na matéria seca (MS das rações isonitrogenadas experimentais. O consumo de MS (1,1, 1,0, 0,9 e 0,9 kg por dia, proteína bruta (199,2, 181,5, 179,0 e 175,2 g por dia e o ganho de peso vivo (298, 275, 280 e 255 g por dia diminuíram linearmente, e o consumo de extrato etéreo (43,8, 49,7, 57,2 e 66,0 g por dia aumentou linearmente com o aumento da participação de GS nas rações. Não houve efeito na conversão alimentar, características e rendimento de cortes da carcaça. A inclusão de GS na ração com alto teor de concentrado proporciona desempenho satisfatório aos cordeiros em confinamento.The objective of this work was to evaluate the effects of raw soybean on lamb performance, carcass yield and lamb cuts. Raw soybean was added at 0, 7, 14 and 21% of the diet dry matter (isonitrogenous. Sixty-four Santa Inês lambs (initial body weight 19.5±0.19 kg and 75±2 days old were assigned to a complete randomized block design according to body weight and age at beginning of the trial. Dry matter intake (1.1, 1.0, 0.9 and 0.9 kg per day, crude protein intake (199.2, 181.5, 179.0 and 175.2 g per day and average daily gain (298, 275, 280, 255 g per day decreased linearly, and ether extract intake (43.8, 49.7, 57.2 and 66.0 g per day increased linearly, as levels of raw soybean increased. Feed conversion, carcass yield and lamb cuts were not affected by raw soybean inclusion in the diet. The inclusion of raw soybean in high concentrate diets provides satisfactory feedlot lamb performance.

  6. Análise da variabilidade da frequência cardíaca em cordeiros da raça Bergamácia, do nascimento aos 35 dias de idade

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    K. Koether

    2016-08-01

    Full Text Available RESUMO A atividade do sistema nervoso autônomo sobre o coração pode ser verificada pela variabilidade da frequência cardíaca (VFC, método que quantifica e assim infere sobre a modulação autonômica cardíaca, refletindo o funcionamento do sistema nervoso autônomo. Durante o período neonatal, diferenças significativas no que se refere à maturação autonômica são descritas em diversas espécies. Embora a espécie ovina venha sendo utilizada como modelo experimental em diversos protocolos em neonatologia e cardiologia em humanos, estudos descritivos sobre a VFC utilizando animais saudáveis e não sedados são escassos na literatura. O objetivo do estudo foi descrever a VFC em cordeiros da raça Bergamácia durante os primeiros 35 dias de idade. Foram realizados exames eletrocardiográficos em 20 cordeiros da raça Bergamácia a partir do nascimento e semanalmente até o 35° dia de idade. A VFC foi analisada pelo intervalo RR normal (batimentos sinusais, pela frequência cardíaca, pelo índice de tônus vasovagal (iTVV, pela raiz quadrada da média do quadrado das diferenças entre intervalos RR normais adjacentes (RMSSD e pela raiz quadrada da somatória do quadrado das diferenças dos valores individuais em relação ao valor médio, dividido pelo número de iR-R em 90 segundos - VFC global (RMSM. Todos os parâmetros se alteraram ao longo das semanas. A frequência cardíaca média elevou-se entre o nascimento e os primeiros sete dias de idade, com decréscimo nas quatro semanas subsequentes, sendo o menor valor encontrado aos 35 dias de idade (145,63±37,80bpm. Entre 21, 28 e 35 dias de idade, o iTVV elevou-se significativamente, o RMSM a partir do 28º dia, e, aos 35 dias, o RMSSD, reflexo da ativação parassimpática, exibiu diferenças em relação aos momentos subsequentes. O início da predominância parassimpática, refletida nos índices da VFC, particularmente o iTVV, ocorre aos 21 dias de idade. A partir dos 35 dias

  7. Natural infection by Eimeria spp. in a cohort of lambs raised extensively in Northeast Brazil Infecção natural por Eimeria spp. em uma criação de cordeiros criados extensivamente no Nordeste do Brasil

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    Rizia Maria da Silva

    2011-06-01

    Full Text Available The aim of the study was to examine and describe the changes in the course of Eimeria infection in a cohort of lambs of the mixed breed Santa Inês raised extensively on a farm in the State of Rio Grande do Norte, northeastern Brazil. The study was carried out between April and August 2008, during which period fecal samples were collected on a weekly basis from each of the 27 male lambs starting from the day after birth until the age of 90 days. Samples were analyzed under optical microscope and those testing positive for Eimeria oocysts were submitted to a quantitative analysis. Oocysts were detected in 17% of the lambs by week 3, but by week 6 100% of the animals were infected. Eight species of Eimeria were identified in the fecal samples, namely, in decreasing order of prevalence, E. crandallis, E. parva, E. granulosa, E. ovinoidalis, E. ahsata, E. ovina, E. faurei and E. intricata. Of the 191 fecal samples that contained Eimeria oocysts, only 32 (16.8% were infected with a single species whereas 23 (12.0% were infected with at least two species and 136 (71.2% harbored three or more species. Although Eimeria coccidiosis is a complex disease owing to the mixed nature of the infective agents, an ongoing prevention program should be implemented to reduce production losses.O objetivo do estudo foi analisar e descrever as alterações no curso da infecção por Eimeria em uma criação de cordeiros mestiços da raça Santa Inês criados extensivamente em uma fazenda no Estado do Rio Grande do Norte, nordeste do Brasil. O estudo foi realizado entre abril e agosto de 2008, período durante o qual amostras fecais foram coletadas semanalmente de 27 cordeiros machos a partir do nascimento até a idade de 90 dias. As amostras foram analisadas em microscópio óptico e aquelas positivas para oocistos de Eimeria foram submetidos a uma análise quantitativa. Oocistos foram detectados em 17% dos cordeiros na terceira semana, mas na sexta semana 100% dos

  8. Desempenho de cordeiros alimentados com silagem de girassol ou de milho com proporções crescentes de ração concentrada Performance of sheep fed sunflower silage or corn silage with increasing proportion of commercial concentrate

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    Mauro Sartori Bueno

    2004-12-01

    Full Text Available Foram realizados dois experimentos com o objetivo de avaliar o valor nutritivo de dietas à base de silagens de milho ou de girassol e o desempenho de ovinos alimentados com estas dietas acrescidas de níveis crescentes de concentrado comercial (20, 40 e 60%. Para avaliação do valor nutritivo e dos coeficientes de digestibilidade aparente dos nutrientes, utilizou-se delineamento em esquema fatorial (2x3, duas silagens e três proporções de ração comercial, com três ovinos por tratamento. Para avaliação do desempenho de cordeiros, o ensaio foi em blocos ao acaso, em esquema fatorial 2x3 (duas silagens e três proporções de ração comercial, com cinco cordeiros por tratamento. Os coeficientes de digestibilidade aparente de MS, MO, FB, ENN, FDN, FDA e de celulose foram menores para as dietas à base de silagem de girassol. As dietas com silagem de milho apresentaram maiores valores de ingestão diária de matéria seca (709,5 x 609,7 g e ganho diário de peso vivo (181,8 x 108,2 g e menores de conversão alimentar (3,82 x 5,35 kg de MS/kg de ganho de PV que as de girassol. As dietas à base de silagem de girassol apresentaram valor nutritivo inferior às de silagem de milho, o que acarretou pior desempenho dos cordeiros. Os animais alimentados com dietas à base de silagem de girassol necessitam de maior quantidade de ração concentrada para obterem desempenho similar aos alimentados com silagem de milho.Two experiments were conduct to evaluate the effect of dietary nutritive value and performance of sheep fed corn- or sunflower silage-based diet with increasing concentrate proportion (20, 40 and 60%. A factorial design (2x3 was used to evaluate nutritive value and digestibility coefficient of two silages with three concentrate levels and three sheep for each treatment. For lamb performance, a randomized block design in a factorial arrangement (2x3 was used to evaluate lamb performance, with five Suffolk lambs/treatment. Apparent

  9. Idade de desmame de cordeiros deslanados para terminação em confinamento, no litoral norte da Bahia Weaning age on fedlot hair sheep lambs performance in the northern litoral of Bahia

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    Davi Correia de Freitas

    2005-08-01

    Full Text Available Trinta e dois cordeiros (16 machos e 16 fêmeas deslanados mestiços de Santa Inês, criados com as matrizes em pastagem de Brachiaria humidicola e suplementados em creep-feeding no período noturno, foram distribuídos em delineamento inteiramente casualizado, em esquema fatorial 4x2 - quatro idades de desmame (56, 70, 84 e 98 dias e sexo, com o objetivo de determinar a melhor idade para o desmame desses animais. Ao desmame, os cordeiros foram confinados, até completarem 126 dias de vida, em baias individuais, onde receberam feno de Tifton 85 (Cynodon spp. cv Tifton 85, água e sal mineral ad libitum e ração concentrada na proporção de 2% do peso vivo. Houve efeito significativo da interação dos fatores idade de desmame e sexo sobre GPC e GPD, em que os cordeiros desmamados aos 84 dias foram superiores às cordeiras desmamadas com a mesma idade. Não se observou efeito significativo na interação dos fatores idade de desmame e sexo sobre GPND e CAC. Verificou-se efeito quadrático da idade de desmame para as variáveis GPND, GPD e CAC. Não se observou efeito significativo do sexo em nenhum dos parâmetros avaliados. A idade de desmame de 76 dias proporcionou maximização dos parâmetros GPND e GPD, enquanto a CAC mais eficiente foi observada nos animais desmamados aos 72 dias.Thirty-two crossbred Santa Inês hair sheep lambs (16 males and 16 females bred with their female progenitors on pasture of Brachiaria humidicola grass, supplemented in creep-feeding during the night, were allotted to a completely randomized design, in a factorial arrangement 4 x 2, four weaning ages (56, 70, 84 and 98 days and sex to determine the best weaning age. At weaning, the lambs were confined in individual pens until 126 days old, when were daily fed Tifton 85 hay, water and mineral salt ad libitum and concentrate diet in the proportion of 2% body weight. There was a significant effect of weaning age vs sex interaction on DWC and DWG, where the males

  10. Polpa cítrica em rações para cordeiros em confinamento: características da carcaça e qualidade da carne Citrus pulp in diets for feedlot lambs: carcass characteristics and meat quality

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    Gustavo Henrique Rodrigues

    2008-10-01

    Full Text Available Objetivou-se avaliar os efeitos do fornecimento de polpa cítrica na dieta sobre as características de carcaça e a qualidade da carne de cordeiros em confinamento. Utilizaram-se 32 cordeiros Santa Inês distribuídos em delineamento de blocos completos casualizados com quatro tratamentos e oito repetições, os quais foram definidos pelo peso e pela idade dos animais no início do experimento de desempenho. Os animais foram alimentados com rações contendo 90% de concentrado (milho moído e/ou polpa cítrica, farelo de soja e minerais e 10% de feno de coastcross (Cynodon spp. A polpa cítrica foi adicionada nos níveis 23,7; 46,1 e 68,4% da MS em substituição a 33, 67 e 100% do milho. Ao atingirem 33 kg de peso corporal médio, os cordeiros foram abatidos para avaliação dos rendimentos de carcaça quente e fria, da perda por resfriamento, da espessura de gordura de cobertura, da área de olho-de-lombo, dos rendimentos de cortes e da proporção músculo:gordura:osso, além da capacidade de retenção de água, da cor, da perda de peso por cozimento e do pH da carne. As características de carcaça não foram alteradas pela substituição parcial ou total do milho por polpa cítrica. Entretanto, a substituição total do milho por polpa cítrica reduziu em 12,4% o teor de gordura na carcaça.The objective of this trial was to determine the effects of feeding diets containing citrus pulp on carcass characteristics and meat quality of feedlot lambs. Thirty-two Santa Ines lambs were distributed in a complete randomized block design according to body weight and age at the beginning of the performance trial. Lambs were fed diets containing 90% concentrate (corn and/or citrus pulp, soybean meal and minerals and 10% coastcross hay (Cynodon spp. Citrus pulp was added at levels 23.7, 46.1 and 68.4% in the DM, replacing corn by 33, 67 or 100%. When lambs reached 33 kg of BW, they were slaughtered to determine dressing percentage, cold carcass yield

  11. Características de carcaça de cordeiros Ideal e cruzas Border Leicester X Ideal submetidos a três sistemas alimentares Carcass characteristics of Polwarth and Border Leicester crossbred lambs in three feed systems

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    Henrique Silla Lopes de Almeida

    2006-10-01

    Full Text Available O experimento foi realizado com intuito de avaliar o efeito do cruzamento entre as raças Ideal e Border Leicester sobre as características da carcaça de cordeiros submetidos a distintos sistemas alimentares. Foram utilizados 48 cordeiros, machos não castrados, desmamados em média aos 60 dias de idade, sendo: 16 da raça Ideal (I, 16 cruzados ½ Border Leicester ½ Ideal (BI e 16 cruzados ¾ Border Leicester ¼ Ideal (BBI, aleatoriamente distribuídos em três sistemas de alimentação: pastagem cultivada (PC, pastagem cultivada + suplementação (PCS e pastagem natural + suplementação (PNS. O abate ocorreu quando os animais atingiram 65% do peso vivo adulto de seu grupo genético. Houve interação significativa entre genótipos e sistemas de alimentação somente para a variável peso de costela. Foi verificado efeito significativo do cruzamento para as variáveis peso de carcaça quente (PCQ, rendimento de carcaça quente (RCQ, peso de carcaça fria (PCF, rendimento de carcaça fria (RCF, área de olho de lombo (AOL, pesos de paleta (PAL e peso perna (PER. O cruzamento entre as raças Border Leicester e Ideal resultou em pesos e rendimentos de carcaça superiores e redução da deposição de gordura nas carcaças.The experiment was carried out to study the effect of crossing Border Leicester and Polwarth breeds on carcass characteristics of lambs submitted to different feed systems. Forty-eight lambs, non-castrate males, weaned averaging 60 days of age were used: 16 Polwarth (P, 16 ½ Border Leicester ½ Polwarth (BP and 16 ¾ Border Leicester ¼ Ideal (BBP. Animals were randomly distributed in three feed systems: cultivated pasture (CP, cultivated pasture + supplementation (CPS and natural pasture + supplementation (NPS. The lambs were slaughtered when they reached 65% of the adult live weight of their genetic groups. Genotype X feed systems interaction was observed only for rib weight. It was verified significant effect of the

  12. Influência da raça, sexo e peso/idade sobre o rendimento da carcaça em cordeiros The influence of breed, sex and weight/age on carcass yield in lambs

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    Maria Teresa Moreira Osório

    1999-03-01

    Full Text Available O estudo objetivou quantificar e comparar o rendimento da carcaça em cordeiros machos e fêmeas, abatidos com 63-73 dias de idade (peso de carcaça fria entre 6,5 kg e 7,9 kg e 80-90 dias de idade (peso de carcaça fria entre 8,0 kg e 9,5 kg, procedentes das raças Rasa Aragonesa, Ojinegra de Teruel e Roya Bilbilitana. Não foi verificada diferença de rendimentos de carcaça entre as raças; por outro lado, as fêmeas apresentaram rendimentos superiores aos machos; assim como os cordeiros de maior idade/peso de carcaça apresentaram rendimentos superiores aos de menor idade/peso de carcaça. As raças que participam da denominação específica de qualidade "Ternasco de Aragón" (Rasa Aragonesa, Ojinegra de Teruel e Roya Bilbilitana apresentam rendimentos de carcaça semelhantes. Entretanto, o sexo e a idade/peso de carcaça são fatores de variação do rendimento de carcaça que devem ser considerados para uma uniformização e comercialização de um produto de qualidade.This study aimed to compare and quantify carcass yield of male and female lambs of the following breeds: Rasa Aragonesa, Ojinegra de Teruel and Roya Bilbilitana. Animals were slaughtered, one group at 63-73 days of age (cool carcass weight between 6.5 and 7.3 kg and another when 80-90 days of age (cool carcass weight between 8.0 and 9.5 kg. Carcass yield has not been influenced by breed. On the other hand, females have shown yields higher than the males; as well as lambs of higher age/weight of carcass did show higher yields than those of lower age/weight of carcass. These breeds, which comprise the ones that receive the specific denomination for quality "Ternasco de Aragón", show similar carcass yields. However, sex and age/weight of carcass are variation factors of carcass yields which should be considered for a standardization and selling of a quality product.

  13. Apparent digestibility of diets with combinations of soybean hulls and coastcross (Cynodon sp. hay offered to ram lambs Digestibilidade aparente de dietas com combinações de casca de soja e feno de "coastcross" (Cynodon sp. oferecidas para cordeiros

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    Rafael Canonenco de Araujo

    2008-12-01

    Full Text Available Soybean hulls (SH are an alternative fiber source that may be used to maintain neutral detergent fiber (NDF concentration while increasing the energy concentration of ruminant diets. The objective of this experiment was to determine the effects of replacing coastcross (Cynodon sp. hay NDF by SH NDF on the apparent digestibility of nutrients and nitrogen balance of Santa Inês ram lambs. Twenty-four animals (42.5 ± 3.6 kg of body weight and six months old were placed in metabolism crates and assigned in a randomized complete block design defined by body weight (BW. Experimental diets provided a similar concentration of NDF (52% and crude protein (15%. Hay NDF from a 70% roughage-based diet was replaced with SH NDF by 33%, 67%, and 100%, resulting in 0, 25, 52, and 77% of SH in the dietary dry matter (DM, respectively. There was a linear increase (p 0.05 on water intake when SH replaced hay. The SH can replace forage and may be included up to 77% in the dietary DM of ram lambs with satisfactory values of nutrient digestibilities.A casca de soja (CS é uma fonte de fibra alternativa que visa manter o teor de fibra em detergente neutro (FDN e aumentar a concentração energética da dieta de ruminantes. O objetivo deste experimento foi avaliar os efeitos da substituição da FDN de feno de "coastcross" (Cynodon sp. pela FDN da CS sobre a digestibilidade aparente dos nutrientes e balanço de nitrogênio em cordeiros Santa Inês. Vinte e quatro animais (42,5 ± 3,6 kg de peso vivo e seis meses de idade foram colocados em gaiolas para ensaio de digestibilidade e arranjados em delineamento blocos completos casualizados definidos pelo peso vivo (PV. As dietas isonitrogenadas (15% de proteína bruta continham concentrações semelhantes de FDN (52%. O tratamento controle foi composto de 70% de feno na matéria seca (MS da dieta, sendo a FDN proveniente do feno substituída em 33%, 67% e 100% pela FDN proveniente da CS, correspondendo a 0, 25, 52 e 77% de

  14. Desempenho de cordeiros alimentados com dietas contendo sal forrageiro de espécies vegetais xerófitas Performance of lambs fed diets with fodder salt composed of xerophilic plants species

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    Geógenes da Silva Gonçalves

    2008-12-01

    Full Text Available Este trabalho foi realizado com o objetivo de avaliar o uso de sal forrageiro sobre os consumos de sal forrageiro (CSF e de feno de capim-pangola (Digitaria decumbens e os consumos de matéria seca (MS, proteína bruta (PB, fibra em detergente neutro (FDN, hemicelulose (HCEL, lignina e água (AGU, além do ganho de peso diário (GPD e da conversão alimentar de cordeiros em confinamento. Os sais forrageiros foram compostos de farelos de fenos (90% das dicotiledôneas, sal mineral (5% e milho triturado (5%. Utilizaram-se 30 animais machos não-castrados, mestiços Santa Inês, distribuídos em delineamento inteiramente casualizado, com seis tratamentos (sal mineral; sal forrageiro de leucena, Leucaena leucocephala; sal forrageiro da parte aérea de mandioca, Manihot esculenta; sal forrageiro de feijão-bravo, Macroptilium bracteatum; sal forrageiro de barriguda, Ceiba samauma; e sal forrageiro de quipé, Piptadenia moniliformis, cada um com cinco repetições. Os sais forrageiros de leucena e da parte aérea de mandioca promoveram melhores resultados de desempenho, ganhos de pesos totais e conversão alimentar, o que evidencia o potencial dessas forrageiras para formulação de sal forrageiro, utilizado na suplementação de dietas para cordeiros em confinamento.This study was to evaluate the use of fodder salt (salt and dicotyledon hay mix on daily intake of fodder salt (IFS and pangola (Digitaria decumbens hay, and intakes of dry matter (DM, crude protein (CP, neutral detergent fiber (NDF, hemicellulose (HCEL, lignin and water (AGU, in addition to daily weight gain (ADG and feed conversion tatio of lambs in confinement. Fodder salts were compound by dicotyledon hay meal (90%, mineral salt (5% and ground maize (5%. Thirty non-castrated male animals, crossbred Santa Inez, were distributed to a completely randomized design, with six fodder salts (mineral salt, fodder salts of: leucaena, (Leucaena leucocephala; aerial part of cassava, (Manihot

  15. The Inter-Eruption Timescale of Classical Novae from Expansion of the Z Camelopardalis Shell

    CERN Document Server

    Shara, Michael M; Zurek, David; Martin, Christopher D; Neill, James D; Seibert, Mark

    2012-01-01

    The dwarf nova Z Camelopardalis is surrounded by the largest known classical nova shell. This shell demonstrates that at least some dwarf novae must have undergone classical nova eruptions in the past, and that at least some classical novae become dwarf novae long after their nova thermonuclear outbursts. The current size of the shell, its known distance, and the largest observed nova ejection velocity set a lower limit to the time since Z Cam's last outburst of 220 years. The brightest part of the Z Cam shell's radius is currently p ~ 1690 pixels. No expansion of the radius of the brightest part of the ejecta was detected, with an upper limit of pdot 5,000 years ago. However, including the important effect of deceleration as the ejecta sweeps up interstellar matter in its snowplow phase reduces the lower limit to 1300 years. This is the first strong test of the prediction of nova thermonuclear runaway theory that the inter-outburst times of classical novae are longer than 1000 yr. The intriguing suggestion ...

  16. SWIFT X-RAY OBSERVATIONS OF CLASSICAL NOVAE. II. THE SUPER SOFT SOURCE SAMPLE

    Energy Technology Data Exchange (ETDEWEB)

    Schwarz, Greg J. [American Astronomical Society, 2000 Florida Avenue, NW, Suite 400, Washington, DC 20009-1231 (United States); Ness, Jan-Uwe [XMM-Newton Science Operations Centre, ESAC, Apartado 78, 28691 Villanueva de la Canada, Madrid (Spain); Osborne, J. P.; Page, K. L.; Evans, P. A.; Beardmore, A. P. [Department of Physics and Astronomy, University of Leicester, Leicester LE1 7RH (United Kingdom); Walter, Frederick M. [Department of Physics and Astronomy, Stony Brook University, Stony Brook, NY 11794-3800 (United States); Andrew Helton, L. [SOFIA Science Center, USRA, NASA Ames Research Center, M.S. N211-3, Moffett Field, CA 94035 (United States); Woodward, Charles E. [Minnesota Institute of Astrophysics, 116 Church Street S.E., University of Minnesota, Minneapolis, MN 55455 (United States); Bode, Mike [Astrophysics Research Institute, Liverpool John Moores University, Birkenhead CH41 1LD (United Kingdom); Starrfield, Sumner [School of Earth and Space Exploration, Arizona State University, P.O. Box 871404, Tempe, AZ 85287-1404 (United States); Drake, Jeremy J., E-mail: Greg.Schwarz@aas.org [Smithsonian Astrophysical Observatory, 60 Garden Street, MS 3, Cambridge, MA 02138 (United States)

    2011-12-01

    The Swift gamma-ray burst satellite is an excellent facility for studying novae. Its rapid response time and sensitive X-ray detector provides an unparalleled opportunity to investigate the previously poorly sampled evolution of novae in the X-ray regime. This paper presents Swift observations of 52 Galactic/Magellanic Cloud novae. We included the X-Ray Telescope (0.3-10 keV) instrument count rates and the UltraViolet and Optical Telescope (1700-8000 A) filter photometry. Also included in the analysis are the publicly available pointed observations of 10 additional novae the X-ray archives. This is the largest X-ray sample of Galactic/Magellanic Cloud novae yet assembled and consists of 26 novae with Super Soft X-ray emission, 19 from Swift observations. The data set shows that the faster novae have an early hard X-ray phase that is usually missing in slower novae. The Super Soft X-ray phase occurs earlier and does not last as long in fast novae compared to slower novae. All the Swift novae with sufficient observations show that novae are highly variable with rapid variability and different periodicities. In the majority of cases, nuclear burning ceases less than three years after the outburst begins. Previous relationships, such as the nuclear burning duration versus t{sub 2} or the expansion velocity of the eject and nuclear burning duration versus the orbital period, are shown to be poorly correlated with the full sample indicating that additional factors beyond the white dwarf mass and binary separation play important roles in the evolution of a nova outburst. Finally, we confirm two optical phenomena that are correlated with strong, soft X-ray emission which can be used to further increase the efficiency of X-ray campaigns.

  17. Psicologia Positiva: uma nova abordagem para antigas questões

    Directory of Open Access Journals (Sweden)

    Simone dos Santos Paludo

    2007-04-01

    Full Text Available Historicamente, a Psicologia preocupou-se em investigar patologias, negligenciado os aspectos saudáveis dos seres humanos. Mas, a partir de 1998, assumindo a presidência da American Psychological Association, Seligman iniciou movimento denominado Psicologia Positiva, que visa oferecer nova abordagem às potencialidades e virtudes humanas, estudando as condições e processos que contribuem para a prosperidade dos indivíduos e comunidades. Este artigo apresenta e discute essa nova proposta científica, que promete melhorar a qualidade de vida dos indivíduos e prevenir patologias; também as lacunas existentes nas investigações em Ciências Humanas, as contribuições teóricas e empíricas e as possíveis aplicações desse conhecimento.

  18. Nocardia nova mycetoma over forehead in a lepromatous leprosy patient.

    Science.gov (United States)

    Dhingra, M; Kaistha, N; Bansal, N; Solanki, L S; Chander, J; Thami, G P; van de Sande, W W

    2012-07-15

    We present a case of a 31-year-old male, a known patient with lepromatous leprosy with a type 2 lepra reaction, who presented with a slowly growing asymptomatic swelling with multiple discharging sinuses over the forehead that developed over 6 months. Smears of the serosanguinous discharge on Gram staining showed Gram-positive branching filamentous bacilli, which on culture on blood agar showed chalky-white colonies. Histology of the lesion showed suppurative granulomas with polymorphs surrounding characteristic grains. The isolate was identified as Nocardia nova by gene sequencing and the patient was started on combined antibiotic therapy that resulted in complete resolution of the infection in six months. To the best of our knowledge, this is the first report of mycetoma related to Nocardia nova in association with leprosy.

  19. Message Correlation Analysis Tool for NOvA

    CERN Document Server

    CERN. Geneva

    2012-01-01

    A complex running system, such as the NOvA online data acquisition, consists of a large number of distributed but closely interacting components. This paper describes a generic realtime correlation analysis and event identification engine, named Message Analyzer. Its purpose is to capture run time abnormalities and recognize system failures based on log messages from participating components. The initial design of analysis engine is driven by the DAQ of the NOvA experiment. The Message Analyzer performs filtering and pattern recognition on the log messages and reacts to system failures identified by associated triggering rules. The tool helps the system maintain a healthy running state and to minimize data corruption. This paper also describes a domain specific language that allows the recognition patterns and correlation rules to be specified in a clear and flexible way. In addition, the engine provides a plugin mechanism for users to implement specialized patterns or rules in generic languages such as C++.

  20. VERITAS OBSERVATIONS OF THE NOVA IN V407 CYGNI

    Energy Technology Data Exchange (ETDEWEB)

    Aliu, E. [Department of Physics and Astronomy, Barnard College, Columbia University, NY 10027 (United States); Archambault, S. [Physics Department, McGill University, Montreal, QC H3A 2T8 (Canada); Arlen, T. [Department of Physics and Astronomy, University of California, Los Angeles, CA 90095 (United States); Aune, T.; Bouvier, A. [Santa Cruz Institute for Particle Physics and Department of Physics, University of California, Santa Cruz, CA 95064 (United States); Beilicke, M.; Buckley, J. H.; Bugaev, V.; Dickherber, R. [Department of Physics, Washington University, St. Louis, MO 63130 (United States); Benbow, W. [Fred Lawrence Whipple Observatory, Harvard-Smithsonian Center for Astrophysics, Amado, AZ 85645 (United States); Bradbury, S. M. [School of Physics and Astronomy, University of Leeds, Leeds LS2 9JT (United Kingdom); Byrum, K. [Argonne National Laboratory, 9700 South Cass Avenue, Argonne, IL 60439 (United States); Cannon, A.; Collins-Hughes, E. [School of Physics, University College Dublin, Belfield, Dublin 4 (Ireland); Cesarini, A.; Connolly, M. P. [School of Physics, National University of Ireland Galway, University Road, Galway (Ireland); Ciupik, L. [Astronomy Department, Adler Planetarium and Astronomy Museum, Chicago, IL 60605 (United States); Cui, W. [Department of Physics, Purdue University, West Lafayette, IN 47907 (United States); Decerprit, G. [DESY, Platanenallee 6, 15738 Zeuthen (Germany); Duke, C., E-mail: daniel-d-gall@uiowa.edu, E-mail: kazuma-tsurusaki@uiowa.edu [Department of Physics, Grinnell College, Grinnell, IA 50112-1690 (United States); and others

    2012-07-20

    We report on very high energy (E > 100 GeV) gamma-ray observations of V407 Cygni, a symbiotic binary that underwent a nova outburst producing 0.1-10 GeV gamma rays during 2010 March 10-26. Observations were made with the Very Energetic Radiation Imaging Telescope Array System during 2010 March 19-26 at relatively large zenith angles due to the position of V407 Cyg. An improved reconstruction technique for large zenith angle observations is presented and used to analyze the data. We do not detect V407 Cygni and place a differential upper limit on the flux at 1.6 TeV of 2.3 Multiplication-Sign 10{sup -12} erg cm{sup -2} s{sup -1} (at the 95% confidence level). When considered jointly with data from Fermi-LAT, this result places limits on the acceleration of very high energy particles in the nova.

  1. VERITAS Observations of the Nova in V407 Cygni

    Science.gov (United States)

    Aliu, E.; Archambault, S.; Arlen, T.; Aune, T.; Beilicke, M.; Benbow, W.; Bouvier, A.; Bradbury, S. M.; Buckley, J. H.; Bugaev, V.; Byrum, K.; Cannon, A.; Cesarini, A.; Ciupik, L.; Collins-Hughes, E.; Connolly, M. P.; Cui, W.; Decerprit, G.; Dickherber, R.; Perkins, J. S.

    2012-01-01

    We report on very high energy (E > 100 GeV) gamma-ray observations of V407 Cygni, a symbiotic binary that underwent a nova outburst producing 0.1- 10 GeV gamma rays during 2010 March 10-26. Observations were made with the Very Energetic Radiation Imaging Telescope Array System during 2010 March 19-26 at relatively large zenith angles, due to the position of V407 Cyg. An improved reconstruction technique for large zenith angle observations is presented and used to analyze the data. We do not detect V407 Cygni and place a differential upper limit on the flux at 1.6 TeV of 2.3 10(exp -12) erg/sq cm/s (at the 95% confidence level). When considered jointly with data from Fermi-LAT, this result places limits on the acceleration of very high energy particles in the nova.

  2. VERITAS Observations of the Nova in V407 Cygni

    CERN Document Server

    Aliu, E; Arlen, T; Aune, T; Beilicke, M; Benbow, W; Bouvier, A; Bradbury, S M; Buckley, J H; Bugaev, V; Byrum, K; Cannon, A; Cesarini, A; Ciupik, L; Collins-Hughes, E; Connolly, M P; Cui, W; Decerprit, G; Dickherber, R; Duke, C; Dumm, J; Dwarkadas, V V; Errando, M; Falcone, A; Feng, Q; Finley, J P; Finnegan, G; Fortson, L; Furniss, A; Galante, N; Gall, D; Godambe, S; Griffin, S; Grube, J; Gyuk, G; Hanna, D; Holder, J; Huan, H; Hughes, G; Humensky, T B; Kaaret, P; Karlsson, N; Kertzman, M; Khassen, Y; Kieda, D; Krawczynski, H; Krennrich, F; Lang, M J; Lee, K; Maier, G; Majumdar, P; McArthur, S; McCann, A; Millis, J; Moriarty, P; Mukherjee, R; Nuñez, P D; Ong, R A; Orr, M; Otte, A N; Pandel, D; Park, N; Perkins, J S; Pohl, M; Prokoph, H; Quinn, J; Ragan, K; Reyes, L C; Reynolds, P T; Roache, E; Rose, H J; Ruppel, J; Saxon, D B; Schroedter, M; Sembroski, G H; Skole, C; Smith, A W; Staszak, D; Telezhinsky, I; Tešić, G; Theiling, M; Thibadeau, S; Tsurusaki, K; Tyler, J; Varlotta, A; Vincent, S; Vivier, M; Wakely, S P; Ward, J E; Weekes, T C; Weinstein, A; Weisgarber, T; Welsing, R; Williams, D A; Zitzer, B

    2012-01-01

    We report on very high energy (E > 100 GeV) gamma-ray observations of V407 Cygni, a symbiotic binary that underwent a nova outburst producing 0.1-10 GeV gamma rays during 2010 March 10-26. Observations were made with the Very Energetic Radiation Imaging Telescope Array System during 2010 March 19-26 at relatively large zenith angles, due to the position of V407 Cyg. An improved reconstruction technique for large zenith angle observations is presented and used to analyze the data. We do not detect V407 Cygni and place a differential upper limit on the flux at 1.6 TeV of 2.3 \\times 10^(-12) erg cm^(-2) s^(-1) (at the 95% confidence level). When considered jointly with data from Fermi-LAT, this result places limits on the acceleration of very high energy particles in the nova.

  3. Morpho-Kinematical Modelling of Nova Eridani 2009 (KT Eri)

    CERN Document Server

    Ribeiro, V A R M; Darnley, M J; Barnsley, R M; Munari, U; Harman, D J

    2013-01-01

    Modelling the morphology of a nova outburst provides valuable information on the shaping mechanism in operation at early stages following the outburst. We performed morpho-kinematical studies, using {\\sc shape}, of the evolution of the H\\alpha\\ line profile following the outburst of the nova KT Eridani. We applied a series of geometries in order to determine the morphology of the system. The best fit morphology was that of a dumbbell structure with a ratio between the major to minor axis of 4:1, with an inclination angle of 58$^{+6}_{-7}$ degrees and a maximum expansion velocity of 2800$\\pm$200 km/s. Although, we found that it is possible to define the overall structure of the system, the radial density profile of the ejecta is much more difficult to disentangle. Furthermore, morphology implied here may also be consistent with the presence of an evolved secondary as suggested by various authors.

  4. Nietzsche e a perspectiva de uma nova ética

    Directory of Open Access Journals (Sweden)

    Vânia Dutra de Azevedo

    2009-07-01

    Full Text Available http://dx.doi.org/10.5007/1677-2954.2009v8n1p85Este artigo apresenta as possibilidades de uma nova perspectiva ética a partir do pensamento de Nietzsche.Essa nova ética tem como especifi cidade o fato de considerar as determinações profundas não conscientescomo prioritárias na defi nição do agir e por entender as éticas como construções explicativas e imposiçõesde uma dada interpretação que remetem a impulsos, forças e vontades de potência.

  5. The Thermonuclear Runaway and the Classical Nova Outburst

    CERN Document Server

    Starrfield, S; Hix, W R

    2016-01-01

    Nova explosions occur on the white dwarf component of a Cataclysmic Variable binary stellar system that is accreting matter lost by its companion. When sufficient material has been accreted by the white dwarf, a thermonuclear runaway occurs and ejects material in what is observed as a Classical Nova explosion. We describe both the recent advances in our understanding of the progress of the outburst and outline some of the puzzles that are still outstanding. We report on the effects of improving both the nuclear reaction rate library and including a modern nuclear reaction network in our one-dimensional, fully implicit, hydrodynamic computer code. In addition, there has been progress in observational studies of Supernovae Ia with implications about the progenitors and we discuss that in this review.

  6. Nova Centauri 2013 = PNV J13544700-5909080

    Science.gov (United States)

    Waagen, Elizabeth O.

    2013-12-01

    Announces the discovery of V1369 Cen = Nova Cen 2013 = PNV J13544700-5909080 by John Seach (Chatsworth Island, NSW, Australia) at unfiltered magnitude 5.5 on 2013 December 02.692 UT. Low-resolution spectra obtained by Locke on Dec. 03.3776 UT and by Kaufman on Dec. 03.621 UT show strong Ha and Hb emission lines, indicating the object is a nova. Announced on IAU CBAT Central Bureau Electronic Telegram 3732 (Daniel W. E. Green, ed.). Finder charts with sequences may be created using the AAVSO Variable Star Plotter (http://www.aavso.org/vsp). Observations should be submitted to the AAVSO International Database. See full Alert Notice for more details and observations.

  7. Equation of state measurements of hydrogen isotopes on Nova

    Energy Technology Data Exchange (ETDEWEB)

    Collins, G.W.; Celliers, P.; Da Silva, L.B.; Cauble, R.; Gold, D.; Foord, M.; Budil, K.S.; Stewart, R.; Holmes, N.C.; Ross, M.; Hammel, B.A.; Kilkenny, J.D.; Wallace, R.J. [Lawrence Livermore National Laboratory, Livermore, California94550 (United States); Ng, A. [University of British Columbia, Vancouver, British Columbia (Canada)

    1998-05-01

    The Nova laser [E. M. Campbell, Laser Part. Beams {bold 9}, 209 (1991)] was used to shock-compress liquid deuterium and obtain new principal Hugoniot measurements of density and pressure between 0.3 and 2.1 Mbar. In this pressure-density region, deuterium is predicted to transform from a molecular insulating fluid to an atomic conducting fluid. Nova data show a rapid increase in density from 0.6 g/cc at 0.3 Mbar, to 1 g/cc at 0.6 Mbar, suggestive of such a transition. The observed sixfold compression near 1 Mbar is larger than predicted by many widely used equation of state models.

  8. Thermal stability and nova cycles in permanent superhump systems

    CERN Document Server

    Retter, A

    2000-01-01

    Archival data on permanent superhump systems are compiled to test the thermal stability of their accretion discs. We find that their discs are almost certainly thermally stable as expected. This result confirms Osaki's suggestion (1996) that permanent superhump systems form a new subclass of cataclysmic variables (CVs), with relatively short orbital periods and high mass transfer rates. We note that if the high accretion rates estimated in permanent superhump systems represent their mean secular values, then their mass transfer rates cannot be explained by gravitational radiation, therefore, either magnetic braking should be extrapolated to systems below the period gap or they must have mass transfer cycles. Alternatively, a new mechanism that removes angular momentum from CVs below the gap should be invoked. We suggest applying the nova cycle scenarios offered for systems above the period gap to the short orbital period CVs. Permanent superhumps have been observed in the two non-magnetic ex-novae with binary...

  9. Erupting Dwarf Novae in the Large Magellanic Cloud

    CERN Document Server

    Shara, M M; Zurek, D R; Shara, Michael M.; Hinkley, Sasha; Zurek, David R.

    2003-01-01

    We report the first likely detections of erupting Dwarf Novae (DN) in an external galaxy: the Large Magellanic Cloud. Six candidates were isolated from approximately a million stars observed every second night over 11 nights with the CTIO 8K x 8K Mosaic2 CCD imager. Artificial dwarf nova and completeness tests suggest that we are seeing only the brightest of the LMC DN, probably SS Cygni-like CVs, but possibly SU UMa-type cataclysmics undergoing superoutbursts. We derive crude but useful limits on the LMC DN surface density, and on the number of DN in the LMC. Many thousands of cataclysmic variables in the Magellanic Clouds can be discovered and characterized with 8 meter class telescopes.

  10. High Energy Neutrino Physics with NOvA

    Energy Technology Data Exchange (ETDEWEB)

    Coan, Thomas [Southern Methodist Univ. , Dallas, TX (United States)

    2016-09-09

    Knowledge of the position of energy deposition in “hit” detector cells of the NOvA neutrino detector is required by algorithms for pattern reconstruction and particle identification necessary to interpret the raw data. To increase the accuracy of this process, the majority of NOvA's 350 000 far detector cell shapes, including distortions, were measured as they were constructed. Using a special laser scanning system installed at the site of the NOvA far detector in Ash River, MN, we completed algorithmic development and measured shape parameters for the far detector. The algorithm and the measurements are “published” in NOνA’s document database (doc #10389, “Cell Center Finder for the NOνA Far Detector Modules”).

  11. Le stelle di Beatrice. Astronomia e astrologia nella "Vita Nova"

    OpenAIRE

    Maraldi, Elisa

    2015-01-01

    Ci sono due luoghi astronomici nella Vita Nova con i quali Dante calcola il tempo in cui si verificano gli episodi principali della storia narrata. Queste nozioni scientifiche contengono implicito un significato astrologico, connesso all’influsso del segno zodiacale dei Gemelli, configurazione astrologica che torna ad ogni anniversario. I Gemelli è il segno zodiacale di Dante, come il poeta afferma nella Commedia: l’invocazione del pellegrino alla costellazione omonima, alla cui influenza egl...

  12. Three new optical nova candidates in M 31

    Science.gov (United States)

    Pietsch, W.; Henze, M.; Burwitz, V.; Kaur, A.; Hartmann, D. H.; Williams, G.; Milne, P.

    2011-06-01

    We report the discovery of three nova candidates in M 31 on 7x60s stacked R filter CCD images obtained with the robotic 60cm telescope with an E2V CCD (2kx2k, 13.5 micron sq. pixels) of the Livermore Optical Transient Imaging System (Super-LOTIS, located at Steward Observatory, Kitt Peak, Arizona, USA) on 2011 June 7.418 UT. The objects are visible on all individual images.

  13. An evaluation of Nova Scotia's alcohol ignition interlock program.

    Science.gov (United States)

    Vanlaar, Ward G M; Mainegra Hing, Marisela; Robertson, Robyn D

    2017-03-01

    Alcohol ignition interlock programs for offenders aim to reduce recidivism among convicted drink drivers. This study presents an evaluation of Nova Scotia's interlock program implemented in 2008 in order to assess its effectiveness to reduce impaired driving and to help identify areas for improvement. Data used include conviction and crash records of individual participants; provincial monthly counts of alcohol-related charges, convictions and fatal and serious crashes; and interlock logged events. Methods used include descriptive statistics, survival analysis, time series and logistic regression analysis. With respect to specific deterrence (i.e., preventing recidivism) there was a 90% reduction in recidivism among voluntary participants since participation in the interlock program and a 79% reduction after these participants exited from the program. With respect to general deterrence (i.e., referring to a preventative effect on the entire population of drivers in Nova Scotia) there were temporary decreases in the numbers of alcohol-related charges (13.32%) and convictions (9.93%) and a small significant decrease in the number of fatal and serious injury alcohol-related crashes, following the implementation of the program. The evidence suggests the interlock program was better at preventing harm due to alcohol-impaired driving than the alternative of not using the interlock program. Recommendations were formulated supporting the continuation of the interlock program in Nova Scotia.

  14. Novae as Tevatrons: Prospects for CTA and IceCube

    CERN Document Server

    Metzger, Brian D; Vurm, Indrek; Beloborodov, Andrei; Bartos, Imre; Vlasov, Andrey

    2015-01-01

    The discovery of novae as sources of ~GeV gamma-rays highlights the key role of shocks and relativistic particle acceleration in these transient systems. Although there is evidence for a spectral cut-off above energies ~1-100 GeV at particular epochs in some novae, the maximum particle energy achieved in these accelerators has remained an open question. The high densities of the nova ejecta (~10 orders of magnitude larger than in supernova remnants) render the gas far upstream of the shock neutral and shielded from ionizing radiation. The amplification of the magnetic field needed for diffusive shock acceleration requires ionized gas, thus confining the acceleration process to a narrow photo-ionized layer immediately ahead of the shock. Based on the growth rate in this layer of the hybrid non-resonant cosmic ray current-driven instability (considering also ion-neutral damping), we quantify the maximum particle energy, Emax, across the range of shock velocities and upstream densities of interest. We find value...

  15. Nova Scotia S-2000 monitoring project. Vol. 1, Performance summary

    Energy Technology Data Exchange (ETDEWEB)

    Makuch, P.; Harrison, S.J. [Queen`s Univ., Kingston, ON (Canada). Solar Calorimetry Lab.

    1994-12-01

    Electric utility companies have increasingly been evaluating and implementing demand management and conservation. As a result there has been growing interest in potential energy savings and capacity benefits of Solar Domestic Hot Water (SDHW) technologies. A computer simulation study showed that SDHW can provide significant savings in hot water heating. Natural Resources Canada through the Canada Centre for Mineral and Energy Technology (CANMET) initiated the S-2000 program. The S-2000 program was initiated to promote cooperation between CANMET, electric utilities and provincial governments interested in determining whether SDHW systems can reduce peak energy demand and pollution emissions. 60 SDHW systems were installed in Nova Scotia. Systems were monitored by Thermo Dynamics Limited and analyzed by the Solar Calorimetry Laboratory at Queen`s University. Results were produced for the monitoring period from October 1993 to August 1994. Results for 32 of the Nova Scotia systems showed winter and summer solar energy supplies of 14.8 MWh and 30 MWh respectively. The system efficiency was determined to be 28.4%. The system performance was consistent with predictions made from computer simulations, with the exception of an unexpectedly severe winter. The solar energy contribution during the winter was lower than that predicted for typical weather conditions. Of the systems monitored daily average hot water use was lower than the reference 239 L/day value. Monitoring of the Nova Scotia systems will continue through 1995 and strategies will be investigated. 15 figs., 5 tables

  16. Shocks in nova outflows. II. Synchrotron radio emission

    CERN Document Server

    Vlasov, Andrey Dmitrievich; Metzger, Brian David

    2016-01-01

    The discovery of GeV gamma-rays from classical novae indicates that shocks and relativistic particle acceleration are energetically key in these events. Further evidence for shocks comes from thermal keV X-ray emission and an early peak in the radio light curve on a timescale of months with a brightness temperature which is too high to result from freely expanding photo-ionized gas. Paper I developed a one dimensional model for the thermal emission from nova shocks. This work concluded that the shock-powered radio peak cannot be thermal if line cooling operates in the post-shock gas at the rate determined by collisional ionization equilibrium. Here we extend this calculation to include non-thermal synchrotron emission. Applying our model to three classical novae, we constrain the amplification of the magnetic field $\\epsilon_B$ and the efficiency $\\epsilon_e$ of accelerating relativistic electrons of characteristic Lorentz factor $\\gamma \\sim 100$. If the shocks are radiative (low velocity $v_{\\rm sh} \\lesssi...

  17. Observational Report of the Classical Nova KT Eridani

    CERN Document Server

    Imamura, Kazuyoshi

    2012-01-01

    A report on the spectroscopic and multi-color photometric observations of high galactic latitude classical nova KT Eridani (Nova Eridani 2009) is presented. After 12.2 days from maximum light, broad and prominent emission lines of Balmer series, He I, He II, N II, N III and O I can be seen on the spectra. The FWHM of H${\\alpha}$ line yields an expansion velocity of approximately 3400 km s$^{-1}$. After 279.4 days from maximum light, we can see prominent emission lines of He II and [O III] on the spectrum. Among them, [O III] (4959, 5007) lines show multiple peaks. From the obtained light curve, KT Eri is classified to be a very fast nova, with a decline rate by two magnitude of $6.2 \\pm 0.3$ days and three of $14.3 \\pm 0.7$ days. We tried to estimate the absolute magnitude ($M_V$) using the Maximum Magnitude versus Rate of Decline relationship and distance of KT Eri. The calculated $M_V$ is approximately -9. Accordingly, the distance and galactic height are approximately 7 kpc and 4 kpc, respectively. Hence, ...

  18. Searching for magnetar powered merger-novae from short GRBs

    CERN Document Server

    Gao, He; Lü, Hou-Jun; Li, Ye

    2016-01-01

    The merger of a double neutron star (NS-NS) binary may result in a rapidly rotating massive NS with an extremely strong magnetic field (i.e., a millisecond magnetar). In this case, the magnetic spin-down of the NS remnant provides an additional source of sustained energy injection, which would continuously power the merger ejecta. The thermal emission from the merger ejecta would give rise to a bright optical "magnetar-powered merger-nova". In this work, we carry out a complete search for magnetar-powered merger-nova from \\emph{Swift} short gamma-ray burst (SGRB) sample. We focus on short GRBs with extended emission or internal plateau, which may signify the presence of magnetars as the central engine. We eventually find three candidates of "magnetar-powered merger-nova" from the late observations of GRB 050724, GRB 070714B and GRB 061006. With standard parameter values, the magentar remnant scenario could well interpret the multi-band data of all three bursts, including the extended emission and their late c...

  19. Spectral Evolution of the Unusual Slow Nova V5558 Sgr

    CERN Document Server

    Tanaka, Jumpei; Fujii, Mitsugu; Ayani, Kazuya; Kato, Taichi; Maehara, Hiroyuki; Kiyota, Seiichiro; Nakajima, Kazuhiro

    2011-01-01

    We report on the spectral evolution of the enigmatic, very slow nova V5558 Sgr, based on the low-resolution spectra obtained at the Fujii-Bisei Observatory and the Bisei Astronomical Observatory, Japan during a period of 2007 April 6 to 2008 May 3. V5558 Sgr shows a pre-maximum halt and then several flare-like rebrightenings, which is similar to another very slow nova V723 Cas. In our observations, the spectral type of V5558 Sgr evolved from the He/N type toward the Fe II type during the pre-maximum halt, and then toward the He/N type again. This course of spectral transition was observed for the first time in the long history of the nova research. In the rebrightening stage after the initial brightness maximum, we could identify many emission lines accompanied by a stronger absorption component of the P-Cygni profile at the brightness maxima. We found that the velocity of the P-Cygni absorption component measured from the emission peak decreased at the brightness maxima. Furthermore, we compared the spectra ...

  20. Direct Three-body Triple-$\\alpha$ in Helium Novae

    CERN Document Server

    Connolly, Ryan; Brown, Edward F

    2016-01-01

    In AM CVn binaries, a white dwarf primary accretes material from a helium-rich white dwarf or stellar companion. The unstable ignition of nuclear burning via the $3\\alpha$ reaction in an accumulated helium layer powers a thermonuclear runaway near accretion rates $\\dot{M} \\lesssim 10^{-6} \\, \\mathrm{M_{\\odot} \\ yr^{-1}}$ that may be observed as helium nova or .Ia supernova. Helium burning in the primary's envelope at temperatures $T \\lesssim 10^{8} \\, \\mathrm{K}$ may proceed via the direct three-body fusion of $\\alpha$-particles. Here we show that the direct three-body rate by Nguyen et al. (2012) -- which is reduced relative to the extrapolated resonant rate at temperatures $T \\gtrsim 5 \\times 10^{7} \\, \\mathrm{K}$ -- results in novae with longer recurrence times and larger ignition masses. By contrast, we find that the enhancement in the direct three-body rate at temperatures below $T \\lesssim 5 \\times 10^{7} \\, \\mathrm{K}$ does not result in significant differences in nova outburst properties. The most mas...

  1. Intial performance from the NOvA surface prototype detector

    Energy Technology Data Exchange (ETDEWEB)

    Muether, M.; /Fermilab

    2011-09-01

    NOvA, the NuMI Off-Axis {nu}{sub e} Appearance experiment, will study {nu}{sub {mu}} {yields} {nu}{sub e} oscillations characterized by the mixing angle {Theta}{sub 13}. Provided {Theta}{sub 13} is large enough, NOvA may ultimately determine the ordering of the neutrino masses and measure CP violation in neutrino oscillations. A complementary pair of detectors will be constructed {approx}14 mrad off beam axis to optimize the energy profile of the neutrinos. This system consists of a surface based 14 kTon liquid scintillator tracking volume located 810 km from the main injector source (NuMI) in Ash River, Minnesota and a smaller underground 222 Ton near detector at the Fermilab. The first neutrino signals at the Ash River Site are expected prior to the 2012 accelerator shutdown. In the meantime, a near detector surface prototype has been completed and neutrinos from two Fermilab sources have been observed using the same highly segmented PVC and liquid scintillator detector system that will be deployed in the full scale experiment. Design and initial performance characteristics of this prototype system are being fed back into the design for the full NOvA program.

  2. Radiative shocks create environments for dust formation in novae

    CERN Document Server

    Derdzinski, Andrea M; Lazzati, Davide

    2016-01-01

    Classical novae commonly show evidence of rapid dust formation within months of the outburst. However, it is unclear how molecules and grains are able to condense within the ejecta given the potentially harsh environment created by ionizing radiation from the white dwarf. Motivated by the evidence for powerful radiative shocks within nova outflows, we propose that dust formation occurs within the cool, dense shell behind these shocks. We incorporate a simple molecular chemistry network and classical nucleation theory with a model for the thermodynamic evolution of the post-shock gas to demonstrate the formation of both carbon and forsterite ($\\rm Mg_2SiO_4$) grains. The high densities due to radiative shock compression ($n \\sim 10^{14}$ cm$^{-3}$) result in CO saturation and rapid dust nucleation. Grains grow efficiently to large sizes $\\gtrsim 0.1\\mu$m, in agreement with IR observations of dust-producing novae, and with total dust masses sufficient to explain massive extinction events such as V705 Cas. As in...

  3. Evolution of Nova TrA 2008 into a High Mass-Accretion Rate Post-Nova

    Science.gov (United States)

    Walter, Frederick M.

    2015-06-01

    NR TrA (Nova TrA 2008) was a normal slow Fe II novae for its first year of evolution. During its third year eclipses appeared, and optical spectra revealed the presence of hot permitted lines of C IV, N V, and O VI in addition to the usual nebular lines. The light curve and spectra resemble those of the V Sge stars. The orbital period is 5.25 hours. The time-resolved spectra show a prominent S-wave in the hot lines with an amplitude of about 100 km/s. We conclude that the system is a CV with a high mass accretion rate that has persisted for some 6 years after the explosion.

  4. RZ Leonis Minoris bridging between ER Ursae Majoris-type dwarf nova and nova-like system

    Science.gov (United States)

    Kato, Taichi; Ishioka, Ryoko; Isogai, Keisuke; Kimura, Mariko; Imada, Akira; Miller, Ian; Masumoto, Kazunari; Nishino, Hirochika; Kojiguchi, Naoto; Kawabata, Miho; Sakai, Daisuke; Sugiura, Yuki; Furukawa, Hisami; Yamamura, Kenta; Kobayashi, Hiroshi; Matsumoto, Katsura; Wang, Shiang-Yu; Chou, Yi; Ngeow, Chow-Choong; Chen, Wen-Ping; Panwar, Neelam; Lin, Chi-Sheng; Hsiao, Hsiang-Yao; Guo, Jhen-Kuei; Lin, Chien-Cheng; Omarov, Chingis; Kusakin, Anatoly; Krugov, Maxim; Starkey, Donn R.; Pavlenko, Elena P.; Antonyuk, Kirill A.; Sosnjvskij, Aleksei A.; Antonyuk, Oksana I.; Pit, Nikolai V.; Baklanov, Alex V.; Babina, Julia V.; Itoh, Hiroshi; Padovan, Stefano; Akazawa, Hidehiko; Kafka, Stella; de Miguel, Enrique; Pickard, Roger D.; Kiyota, Seiichiro; Shugarov, Sergey Yu.; Chochol, Drahomir; Krushevska, Viktoriia; Sekeráš, Matej; Pikalova, Olga; Sabo, Richard; Dubovsky, Pavol A.; Kudzej, Igor; Ulowetz, Joseph; Dvorak, Shawn; Stone, Geoff; Tordai, Tamás; Dubois, Franky; Logie, Ludwig; Rau, Steve; Vanaverbeke, Siegfried; Vanmunster, Tonny; Oksanen, Arto; Maeda, Yutaka; Kasai, Kiyoshi; Katysheva, Natalia; Morelle, Etienne; Neustroev, Vitaly V.; Sjoberg, George

    2016-12-01

    We observed RZ LMi, which is renowned for its extremely short (˜19 d) supercycle and is a member of a small, unusual class of cataclysmic variables called ER UMa-type dwarf novae, in 2013 and 2016. In 2016, the supercycles of this object substantially lengthened in comparison to the previous measurements to 35, 32, and 60 d for three consecutive superoutbursts. We consider that the object virtually experienced a transition to the nova-like state (permanent superhumper). This observed behavior reproduced the prediction of the thermal-tidal instability model extremely well. We detected a precursor in the 2016 superoutburst and detected growing (stage A) superhumps with a mean period of 0.0602(1) d in 2016 and in 2013. Combined with the period of superhumps immediately after the superoutburst, the mass ratio is not as small as in WZ Sge-type dwarf novae, having orbital periods similar to RZ LMi. By using least absolute shrinkage and selection operator (Lasso) two-dimensional power spectra, we detected possible negative superhumps with a period of 0.05710(1) d. We estimated an orbital period of 0.05792 d, which suggests a mass ratio of 0.105(5). This relatively large mass ratio is even above that of ordinary SU UMa-type dwarf novae, and it is also possible that the exceptionally high mass-transfer rate in RZ LMi may be a result of a stripped secondary with an evolved core in a system evolving toward an AM CVn-type object.

  5. Optical spectral evolution of Nova Cygni 1992 = V 1974 Cygni

    Science.gov (United States)

    Rafanelli, P.; Rosino, L.; Radovich, M.

    1995-02-01

    We report the results of the optical spectrophotometric observations of N Cyg 1992 = V 1974 Cyg performed at Asiago between 6 and 670 days after its visual maximum (1992 February 22, mv approximately 4.4). On 1992 February 28, during the first decline the spectrum of the nova was characterized by the presence over a strong continuum of wide emission lines of HI (Balmer), FeII, NaI, CaII, flanked by two systems of P Cyg absorptions with mean radial velocities of -1250 and -1900 km/s. The transition phase was reached at the beginning of April with a gradual fading of the lines of lower ionization potential and the emerging of the HeI, NII, NIII lines. P Cygni absorption features with radial velocity higher than in February were still perceptible. The nova entered the nebular stage some weeks later, at the end of April. The presence in the spectrum, besides (OIII) lambda lambda 4959, 5007, of strong forbidden lines of (NeIII) at lambda lambda 3869, 3968, left no doubt of its classification as a 'neon nova' similar to QU Vul. The evolution of the spectrum in the next months was characterized by the progressive growth of the ionization degree. Following the forbidden lines of (NeIII) and (OIII), also those of (NeIV), (FeVI), (FeVII) and (NeV) became outstanding. The highest degree of ionization was attained on 1993 July, about 500 days from visual maximum, when the coronal lines of (FeX), (FeXI), (AX) reached their highest strength. The steadily decline of the degree of ionization began about one-hundred days later, with the rapid disappearance of the coronal lines and the progressive fading of the lines of highest ionization potential. The intensities of the emission lines during the nova evolution are reported. The discussion concerns the determination of: color excess, absolute magnitude and distance (2.8 kpc) of the nova; effective temperature of the contracting photosphere; and abundance in the ejecta of He, O, N, and Ne, relative to H.

  6. Fermi-LAT detection of the Galactic nova TCP J18102829-2729590

    Science.gov (United States)

    Li, Kwan-Lok; Chomiuk, Laura

    2016-11-01

    Fermi-LAT detection of the Galactic nova TCP J18102829-2729590 Following the discovery of the nova in Sagittarius TCP J18102829-2729590 (CBAT 2016 10 20.383; ATel #9658), we triggered an one-week Fermi ToO (observation number: 090603-1-1; PI: Laura Chomiuk) from 2016-10-25 as part of our Fermi-LAT monitoring campaign for Galactic novae (ATel #9311).

  7. THE INTER-ERUPTION TIMESCALE OF CLASSICAL NOVAE FROM EXPANSION OF THE Z CAMELOPARDALIS SHELL

    Energy Technology Data Exchange (ETDEWEB)

    Shara, Michael M.; Mizusawa, Trisha; Zurek, David [Department of Astrophysics, American Museum of Natural History, Central Park West at 79th Street, New York, NY 10024-5192 (United States); Martin, Christopher D.; Neill, James D. [Department of Physics, Math and Astronomy, California Institute of Technology, 1200 East California Boulevard, Mail Code 405-47, Pasadena, CA 91125 (United States); Seibert, Mark [Observatories of the Carnegie Institution of Washington, 813 Santa Barbara Street, Pasadena, CA 91101 (United States)

    2012-09-10

    The dwarf nova Z Camelopardalis is surrounded by the largest known classical nova shell. This shell demonstrates that at least some dwarf novae must have undergone classical nova eruptions in the past, and that at least some classical novae become dwarf novae long after their nova thermonuclear outbursts. The current size of the shell, its known distance, and the largest observed nova ejection velocity set a lower limit to the time since Z Cam's last outburst of 220 years. The radius of the brightest part of Z Cam's shell is currently {approx}880 arcsec. No expansion of the radius of the brightest part of the ejecta was detected, with an upper limit of {<=}0.17 arcsec yr{sup -1}. This suggests that the last Z Cam eruption occurred {>=}5000 years ago. However, including the important effect of deceleration as the ejecta sweeps up interstellar matter in its snowplow phase reduces the lower limit to 1300 years. This is the first strong test of the prediction of nova thermonuclear runaway theory that the interoutburst times of classical novae are longer than 1000 years. The intriguing suggestion that Z Cam was a bright nova, recorded by Chinese imperial astrologers in October-November 77 B.C.E., is consistent with our measurements. If Z Cam was indeed the nova of 77 B.C.E. we predict that its ejecta are currently expanding at 85 km s{sup -1}, or 0.11 arcsec yr{sup -1}. Detection and measurement of this rate of expansion should be possible in just a few years.

  8. Mortalidade perinatal de cordeiros no semi-árido da Paraíba Perinatal mortality of lambs in the semi-arid region of Paraíba, Brazil

    Directory of Open Access Journals (Sweden)

    Janduí Escarião da Nóbrega Jr

    2005-09-01

    Full Text Available As causas de mortalidade perinatal em ovinos foram estudadas de março de 2002 a outubro 2004 em 27 fazendas da região semi-árida da Paraíba. De 90 cordeiros necropsiados, 41,1% morreram de infecções neonatais, 23,3% por malformações, 10% por inanição/hipotermia, 10% por distocia, 2,2% por predação e 4,4% foram abortos sem causa identificada. Em relação ao momento da morte, 4,4% dos cordeiros morreram antes do parto, 10% durante o parto, 30% no primeiro dia de vida, 20% entre o 2º e 5º dia e 35,6% entre o 4º e 28º dia após o parto. A assistência das ovelhas durante o parto, a desinfecção do umbigo dos cordeiros, a ingestão de colostro 2 a 6 horas após o parto, e a manutenção das ovelhas em locais adequados durante e após o parto contribuiriam para diminuir as mortes perinatais por distocia e infecções neonatais. A alta freqüência de malformações, em diferentes raças, sugere que esses defeitos sejam causados por uma planta tóxica. Os principais defeitos observados foram a flexão permanente dos membros anteriores, braquignatismo, fenda palatina e outras alterações dos ossos da cabeça. Recentemente foi demonstrado o efeito teratogênico de Mimosa tenuiflora ("jurema-preta", uma planta muito comum na região semi-árida, nas áreas de caatinga, que aparentemente é responsável pelas malformações. Os cordeiros mortos por inanição/hipotermia tiveram baixo peso ao nascimento (1,37 ± 0,7kg o que sugere que a principal causa dessas mortes é a deficiente nutrição da mãe durante o último terço da gestação. Considerando-se que na região nordeste, na maioria das fazendas, os carneiros permanecem com as ovelhas durante todo o ano, a adoção de uma estação de monta definida contribuiria para a diminuição da mortalidade perinatal.The causes of perinatal lamb mortality were studied, from March 2002 to October 2004, on 27 farms in the semiarid region of Paraíba, northeastern Brazil. In 90 lambs necropsied

  9. Desempenho de cordeiros inteiros ou submetidos a diferentes métodos de castração abatidos aos 30 kg de peso vivo Performance of intact or submitted to different methods of castration lambs slaughtered at 30 kg of live weight

    Directory of Open Access Journals (Sweden)

    Edson Luis de Azambuja Ribeiro

    2003-06-01

    Full Text Available Foram utilizados neste experimento 31 cordeiros cruzados Hampshire Down, Ile de France e Suffolk, distribuídos em quatro tratamentos: inteiros ou castrados com burdizzo, borracha ou faca. A castração ocorreu aos 58 dias de idade. Após o desmame, aos 84 dias, os animais foram confinados até atingirem o peso vivo de 30 a 32 kg, quando abatidos. Não houve diferença significativa entre os tratamentos e entre os grupos genéticos para os pesos ao nascimento, desmame e abate, para o ganho de peso médio diário do nascimento ao abate e para a idade ao abate. As médias para os ganhos de peso foram 0,179; 0,177; 0,170 e 0,147 kg e para a idade ao abate de 152,0; 156,0; 161,5 e 188,9 dias para os cordeiros inteiros, castrados com burdizzo, com borracha e com faca, respectivamente. Os cordeiros Hampshire Down, Ile de France e Suffolk ganharam, respectivamente, 0,176; 0,163 e 0,166 kg diariamente. Os animais inteiros apresentaram menores rendimentos verdadeiros de carcaça quente ou fria; não havendo outras diferenças importantes entre os tratamentos para as demais características de carcaça estudadas. Os cordeiros Hampshire Down apresentaram maiores rendimentos de carcaça fria, enquanto os Suffolk tiveram menores rendimentos verdadeiros de carcaça e menor percentagem de pescoço, e os Ile de France apresentaram as carcaças mais curtas. O peso ao nascimento teve efeito significativo sobre o ganho de peso e a idade ao abate dos cordeiros. Os resultados mostraram não haver diferenças no desempenho de cordeiros inteiros ou castrados por diferentes métodos abatidos entre 30 e 32 kg de peso vivo, e que pode ocorrer diferenças entre animais de diferentes grupos genéticos quando abatidos com peso semelhante.Thirty-one Hampshire Down, Ile de France and Suffolk crossbred lambs divided into four treatments: intact, castrated with burdizzo, with rubber bands and with knife, were used in this experiment. Castration occurred at 58 days of age. After

  10. Desempenho e características de carcaça de cordeiros das raças Texel, Suffolk e cruza Texel x Suffolk Performance and characteristics of the carcass of lambs the breed Texel, Suffolk and cross Texel x Suffolk

    Directory of Open Access Journals (Sweden)

    Sérgio Carvalho

    2005-10-01

    Full Text Available Este experimento objetivou comparar o desempenho e as características de carcaça de 14 cordeiros, sendo quatro da raça Texel, cinco da raça Suffolk e cinco cruza Texel x Suffolk. Os cordeiros foram desmamados aos 64 dias de idade em média, e terminados em regime de confinamento total, até o abate com idade média de 128 dias. Do nascimento ao desmame, as ovelhas (mães dos cordeiros foram mantidas em pastagem nativa e receberam uma suplementação concentrada na proporção de 1% de peso vivo, tendo também os cordeiros acesso a uma suplementação concentrada na forma de creep-feeding na proporção de 1,5% do peso vivo. O alimento concentrado utilizado na suplementação das ovelhas e dos cordeiros continha 21% de proteína bruta (PB, 70% de nutrientes digestíveis totais (NDT, 2% de cálcio (Ca e 0,4% de fósforo (P. Após o desmame, os cordeiros passaram a receber uma dieta composta por feno de Tifton-85 (Cynodon dactylon + concentrado, na proporção 40:60 na Matéria Seca (MS, a qual continha 15,1% de PB, 60,8% de NDT, 1,4% de Ca e 0,3% de P. O peso ao abate foi inferior (PThe objective of this work was to compare the performance and carcass characteristics of 14 lambs, being four of the Texel, five of the Suffolk and five cross Texel x Suffolk breeds. The lambs were weaned at 64 days of age in average, and finished in feedlot, until slaughtering with average age of 128 days. From birth to weaning, dams were maintained in native pasture and received a concentrated supplementation at a 1% ratio of live weight and lambs had access to a concentrated supplementation in the form of creep-feeding at a 1.5% ratio of the live weight. The concentrated food used in the supplementation of the sheep and the lambs contained 21% of crude protein (CP, 70% of total digestible nutrients (TDN, 2% of calcium (Ca and 0.4% of phosphorus (P. After weaning, lambs started to receive a composed diet of hay made of Tifton-85 (Cynodon dactylon + concentrate

  11. Classical Novae in Andromeda: Light Curves from the Palomar Transient Factory and GALEX

    CERN Document Server

    Cao, Yi; Neill, James D; Kulkarni, S R; Lou, Yu-Qing; Ben-Ami, Sagi; Bloom, Joshua S; Cenko, S Bradley; Law, Nicholas M; Nugent, Peter E; Ofek, Eran O; Poznanski, Dovi; Quimby, Robert M

    2012-01-01

    We present optical light curves of twenty-nine novae in M31 during the 2009 and 2010 observing seasons of the Palomar Transient Factory (PTF). The dynamic and rapid cadences in PTF monitoring of M31, from one day to even ten minutes, provide excellent temporal coverage of nova light curves, enabling us to record the photometric evolution of M31 novae in unprecedented detail. We also detect eight of these novae in the near ultraviolet (UV) band with the Galaxy Evolution Explorer (GALEX) satellite. Novae M31N2009-10b and 2010-11a show prominent UV emission peaking a few days prior to their optical maxima, possibly implying aspherical outbursts. Additionally, our blue-shifted spectrum of the recent outburst of PT And (M31N2010-12a) indicates that it is a recurrent nova in M31 and not a dwarf nova in the Milky Way as was previously assumed. Finally, we systematically searched for novae in all confirmed globular clusters of M31 and found only M31N 2010-10f associated with Bol 126. The specific nova rate in the M31...

  12. CLASSICAL NOVAE IN ANDROMEDA: LIGHT CURVES FROM THE PALOMAR TRANSIENT FACTORY AND GALEX

    Energy Technology Data Exchange (ETDEWEB)

    Cao Yi; Lou Yuqing [Tsinghua Center for Astrophysics (THCA), Department of Physics, Tsinghua University, Beijing 100084 (China); Kasliwal, Mansi M.; Neill, James D.; Kulkarni, S. R.; Quimby, Robert M. [Astronomy Department, California Institute of Technology, 1200 East California Boulevard, Pasadena, CA 91125 (United States); Ben-Ami, Sagi [Department of Particle Physics and Astrophysics, Weizmann Institute of Science, Rehovot 76100 (Israel); Bloom, Joshua S.; Cenko, S. Bradley; Nugent, Peter E. [Department of Astronomy, University of California, Berkeley, CA 94720-3411 (United States); Law, Nicholas M. [Dunlap Institute for Astronomy and Astrophysics, University of Toronto, 50 St. George Street, Toronto, M5S 3H4 Ontario (Canada); Ofek, Eran O. [Benoziyo Center for Astrophysics, Faculty of Physics, Weizmann Institute of Science, Rehovot 76100 (Israel); Poznanski, Dovi, E-mail: ycao@astro.caltech.edu [School of Physics and Astronomy, Tel-Aviv University, Tel Aviv 69978 (Israel)

    2012-06-20

    We present optical light curves of 29 novae in M31 during the 2009 and 2010 observing seasons of the Palomar Transient Factory (PTF). The dynamic and rapid cadences in PTF monitoring of M31, from one day to ten minutes, provide excellent temporal coverage of nova light curves, enabling us to record the photometric evolution of M31 novae in unprecedented detail. We also detect eight of these novae in the near-ultraviolet (UV) band with the Galaxy Evolution Explorer (GALEX) satellite. Novae M31N 2009-10b and M31N 2010-11a show prominent UV emission peaking a few days prior to their optical maxima, possibly implying aspherical outbursts. Additionally, our blueshifted spectrum of the recent outburst of PT And (M31N 2010-12a) indicates that it is a recurrent nova in M31 and not a dwarf nova in the Milky Way as was previously assumed. Finally, we systematically searched for novae in all confirmed globular clusters (GCs) of M31 and found only M31N 2010-10f associated with Bol 126. The specific nova rate in the M31 GC system is thus about one per year, which is not enhanced relative to the rate outside the GC system.

  13. Binary Orbits as the Driver of Gamma-Ray Emission and Mass Ejection in Classical Novae

    Science.gov (United States)

    Chomiuk, Laura; Linford, Justin D.; Yang, Jun; O'Brien, T. J.; Paragi, Zsolt; Mioduszewski, Amy J.; Beswick, R. J.; Cheung, C. C.; Mukai, Koji; Nelson, Thomas

    2014-01-01

    Classical novae are the most common astrophysical thermonuclear explosions, occurring on the surfaces of white dwarf stars accreting gas from companions in binary star systems. Novae typically expel about 10 (sup -4) solar masses of material at velocities exceeding 1,000 kilometers per second.However, the mechanism of mass ejection in novae is poorly understood, and could be dominated by the impulsive flash of thermonuclear energy, prolonged optically thick winds or binary interaction with the nova envelope. Classical novae are now routinely detected at giga-electronvolt gamma-ray wavelengths, suggesting that relativistic particles are accelerated by strong shocks in the ejecta. Here we report high-resolution radio imaging of the gamma-ray-emitting nova V959 Mon. We find that its ejecta were shaped by the motion of the binary system: some gas was expelled rapidly along the poles as a wind from the white dwarf, while denser material drifted out along the equatorial plane, propelled by orbital motion..At the interface between the equatorial and polar regions, we observe synchrotron emission indicative of shocks and relativistic particle acceleration, thereby pinpointing the location of gamma-ray production. Binary shaping of the nova ejecta and associated internal shocks are expected to be widespread among novae, explaining why many novae are gamma-ray emitters.

  14. Desempenho de cordeiros terminados em confinamento, consumindo silagens de milho de grãos com alta umidade ou grãos de milho hidratados em substituição aos grãos de milho seco da dieta

    Directory of Open Access Journals (Sweden)

    Reis Wagner dos

    2001-01-01

    Full Text Available O experimento foi conduzido para avaliar o uso dos grãos de milho em diferentes formas (grãos de milho secos, silagem de grãos de milho hidratado e silagem de grãos de milho úmido sobre o desempenho de cordeiros terminados em confinamento. Foram usados 60 cordeiros (machos e fêmeas, distribuídos aleatoriamente em cinco tratamentos com doze repetições e alimentados com dietas isoprotéicas e isoenergéticas, em diferentes tratamentos: T1 (silagem de grãos de milho hidratados - SMGH, T2 (Grãos de milho seco - GMS, T3 (50% SGMH + 50% GMS, T4 (silagem de grãos de milho úmidos - SGMU e T5 (50% SGMU + 50% GMS. O volumoso utilizado foi feno de aveia. Foram avaliados ganho de peso diário e conversão alimentar aos 28, 56 e 73 dias de confinamento. A dieta com substituição total dos grãos de milho seco por silagem de grãos de milho úmidos apresentou maior ganho de peso aos 73 dias em relação àqueles obtidos aos 56 e 28 dias de confinamento. Este fato pode ser explicado pela melhor digestibilidade apresentada pelas silagens, atribuída à gelatinização que o amido sofre durante o processo. Assim, a silagem de grãos úmidos pode ser usada com eficácia em dietas para cordeiros.

  15. Chandra Discovers Eruption and Pulsation in Nova Outburst

    Science.gov (United States)

    2001-09-01

    NASA's Chandra X-ray Observatory has discovered a giant outburst of X-rays and unusual cyclical pulsing from a white dwarf star that is closely orbiting another star -- the first time either of these phenomena has been seen in X-rays. The observations are helping scientists better understand the thermonuclear explosions that occur in certain binary star systems. The observations of Nova Aquilae were reported today at the "Two Years of Science with Chandra" symposium by an international team led by Sumner Starrfield of Arizona State University. "We found two important results in our Chandra observations. The first was an underlying pulsation every 40 minutes in the X-ray brightness, which we believe comes from the cyclical expansion and contraction of the outer layers of the white dwarf," said Starrfield. "The other result was an enormous flare of X-rays that lasted for 15 minutes. Nothing like this has been seen before from a nova, and we don't know how to explain it." Novas occur on a white dwarf (a star which used up all its nuclear fuel and shrank to roughly the size of the Earth) that is orbiting a normal size star. Strong gravity tides drag hydrogen gas off the normal star and onto the white dwarf, where it can take more than 100,000 years for enough hydrogen to accumulate to ignite nuclear fusion reactions. Gradually, these reactions intensify until a cosmic-sized hydrogen bomb blast results. The outer layers of the white dwarf are then blown away, producing a nova outburst that can be observed for a period of months to years as the material expands into space. "Chandra has allowed us to see deep into the gases ejected by this giant explosion and extract unparalleled information on the evolution of the white dwarf whose surface is exploding," said Jeremy Drake of the Harvard-Smithsonian Center for Astrophysics. The brightening of Nova Aquilae was first detected by optical astronomers in December 1999. "Although this star is at a distance of more than 6

  16. A LIGHT CURVE ANALYSIS OF CLASSICAL NOVAE: FREE-FREE EMISSION VERSUS PHOTOSPHERIC EMISSION

    Energy Technology Data Exchange (ETDEWEB)

    Hachisu, Izumi [Department of Earth Science and Astronomy, College of Arts and Sciences, The University of Tokyo, 3-8-1 Komaba, Meguro-ku, Tokyo 153-8902 (Japan); Kato, Mariko, E-mail: hachisu@ea.c.u-tokyo.ac.jp, E-mail: mariko@educ.cc.keio.ac.jp [Department of Astronomy, Keio University, Hiyoshi, Kouhoku-ku, Yokohama 223-8521 (Japan)

    2015-01-10

    We analyzed light curves of seven relatively slower novae, PW Vul, V705 Cas, GQ Mus, RR Pic, V5558 Sgr, HR Del, and V723 Cas, based on an optically thick wind theory of nova outbursts. For fast novae, free-free emission dominates the spectrum in optical bands rather than photospheric emission, and nova optical light curves follow the universal decline law. Faster novae blow stronger winds with larger mass-loss rates. Because the brightness of free-free emission depends directly on the wind mass-loss rate, faster novae show brighter optical maxima. In slower novae, however, we must take into account photospheric emission because of their lower wind mass-loss rates. We calculated three model light curves of free-free emission, photospheric emission, and their sum for various white dwarf (WD) masses with various chemical compositions of their envelopes and fitted reasonably with observational data of optical, near-IR (NIR), and UV bands. From light curve fittings of the seven novae, we estimated their absolute magnitudes, distances, and WD masses. In PW Vul and V705 Cas, free-free emission still dominates the spectrum in the optical and NIR bands. In the very slow novae, RR Pic, V5558 Sgr, HR Del, and V723 Cas, photospheric emission dominates the spectrum rather than free-free emission, which makes a deviation from the universal decline law. We have confirmed that the absolute brightnesses of our model light curves are consistent with the distance moduli of four classical novae with known distances (GK Per, V603 Aql, RR Pic, and DQ Her). We also discussed the reason why the very slow novae are about ∼1 mag brighter than the proposed maximum magnitude versus rate of decline relation.

  17. LABORATORY ANALYSIS OF PRESOLAR SILICATE STARDUST FROM A NOVA

    Energy Technology Data Exchange (ETDEWEB)

    Leitner, J.; Kodolanyi, J.; Hoppe, P. [Max Planck Institute for Chemistry, Particle Chemistry Department, Hahn-Meitner-Weg 1, D-55128 Mainz (Germany); Floss, C., E-mail: jan.leitner@mpic.de [Laboratory for Space Sciences and Physics Department, Washington University, One Brookings Drive, St. Louis, MO 63130 (United States)

    2012-08-01

    We report the major element as well as the oxygen, magnesium, and silicon isotope composition of a unique presolar silicate grain found in the fine-grained fraction of the Antarctic CR2 chondrite Graves Nunataks 95229. The grain is characterized by an extremely high {sup 17}O/{sup 16}O ratio (6.3 {+-} 0.2 Multiplication-Sign 10{sup -3}) relative to solar values, whereas its {sup 18}O/{sup 16}O ratio is solar within measurement uncertainty. It also shows enrichments in {sup 25,26}Mg and a significant excess in {sup 30}Si relative to solar system compositions, with {delta}{sup 25}Mg = 79 {+-} 21 per mille , {delta}{sup 26}Mg = 70 {+-} 20 per mille , and {delta}{sup 30}Si = 379 {+-} 92 per mille . This isotopic composition is consistent with an origin in the ejecta of a {approx}1.3-1.4 M{sub Sun} ONe nova with large contributions of material from a main-sequence companion star of roughly solar metallicity. However, many details of the stellar source remain undetermined, owing to the uncertainties of current nova nucleosynthesis models. Auger electron spectroscopic analyses identify O, Mg, Si, and Fe as the grain's major constituents. Its (Mg+Fe)/Si atomic ratios are lower than that of olivine and correspond on average to Fe-Mg-pyroxene. A complex texture and heterogeneous major element distribution within the grain attest to condensation under non-equilibrium conditions, which is consistent with the proposed nova origin.

  18. Novae as Tevatrons: prospects for CTA and IceCube

    Science.gov (United States)

    Metzger, B. D.; Caprioli, D.; Vurm, I.; Beloborodov, A. M.; Bartos, I.; Vlasov, A.

    2016-04-01

    The discovery of novae as sources of ˜0.1-1 GeV gamma-rays highlights the key role of shocks and relativistic particle acceleration in these transient systems. Although there is evidence for a spectral cut-off above energies ˜1-100 GeV at particular epochs in some novae, the maximum particle energy achieved in these accelerators has remained an open question. The high densities of the nova ejecta (˜10 orders of magnitude larger than in supernova remnants) render the gas far upstream of the shock neutral and shielded from ionizing radiation. The amplification of the magnetic field needed for diffusive shock acceleration requires ionized gas, thus confining the acceleration process to a narrow photoionized layer immediately ahead of the shock. Based on the growth rate of the hybrid non-resonant cosmic ray current-driven instability (considering also ion-neutral damping), we quantify the maximum particle energy, Emax, across the range of shock velocities and upstream densities of interest. We find values of Emax ˜ 10 GeV-10 TeV, which are broadly consistent with the inferred spectral cut-offs, but which could also in principle lead to emission extending to ≳ 100 GeV accessible to atmosphere Cherenkov telescopes, such as the Cherenkov Telescope Array (CTA). Detecting TeV neutrinos with IceCube is more challenging, although the prospects are improved for a nearby event (≲ kpc) or if the shock power during the earliest, densest phases of the outburst is higher than implied by the GeV light curves, due to downscattering of the gamma-rays within the ejecta.

  19. Recurrent Novae as a progenitor system of Type Ia Supernovae

    Science.gov (United States)

    Hachisu, Izumi; Kato, Mariko

    2002-11-01

    Theoretical light curves of 8 recurrent novae in outburst are modeled to obtain various physical parameters. Light curve calculation includes reflection effects of the companion star and the accretion disk by the photosphere of the white dwarf (WD). We also include a radiation-induced warping instability of the accretion disk in order to reproduce the second peak of T CrB outbursts. The early visual light curves are well reproduced with an expanded WD photosphere of a thermonuclear runaway model on a very massive WD close to the Chandrasekhar mass limit, i.e., MWD = 1.35 - 1.37 Msolar except for CI Aql. The white dwarf mass of CI Aql is estimated to be MWD = 1.2 +/- 0.05 Msolar. Optically thick winds, which blow from the WDs during the outbursts, play a key role in determining the nova duration and the speed of decline because the wind quickly reduces the envelope mass on the WD. Each envelope mass at the optical maximum is estimated, which indicates an average mass accretion rate on to the WDs during the quiescent phase before the last outburst. Although a large part of the envelope mass is blown in the wind, each WD can retain a substantial part of the envelope mass after hydrogen burning ends. Thus, we have obtained net mass-increasing rates of the WDs. These obtained values strongly indicate that the WDs in the recurrent novae have now grown up to near the Chandrasekhar mass limit and will soon explode as a Type Ia supernova if the WDs consist of carbon and oxygen. We have also clarified the reason why only T CrB shows a secondary maximum.

  20. Discovery of an Apparent Nova in M81

    Science.gov (United States)

    Hornoch, K.; Vaduvescu, O.; Gonzalez, A.

    2013-04-01

    We report the discovery of an apparent nova in the M81 galaxy on a co-added 2000-s narrow-band H-alpha CCD image taken with the 2.5-m Isaac Newton Telescope (INT) + WFC at La Palma in ~1.4" seeing on Apr. 5.946 UT. The new object is visible on individual 400-s frames and well visible on the co-added image (see the finding chart linked below), but is not present on numerous narrow-band H-alpha archival images from the INT down to limiting magnitude as faint as H-alpha = 21.7.

  1. Equation of State measurements of hydrogen isotopes on Nova

    Energy Technology Data Exchange (ETDEWEB)

    Collins, G. W., LLNL

    1997-11-01

    High intensity lasers can be used to perform measurements of materials at extremely high pressures if certain experimental issues can be overcome. We have addressed those issues and used the Nova laser to shock-compress liquid deuterium and obtain measurements of density and pressure on the principal Hugoniot at pressures from 300 kbar to more than 2 Mbar. The data are compared with a number of equation of state models. The data indicate that the effect of molecular dissociation of the deuterium into a monatomic phase may have a significant impact on the equation of state near 1 Mbar.

  2. A nova mobilidade populacional: circulação integral

    OpenAIRE

    Lopes, Policarpo

    1998-01-01

    A mundialização crescente dos mercados, da informação, do turismo e da chamada circulação integral veio dar uma nova amplitude e consistência ao regime de mobilidade generalizada à escala planetária. Os movimentos de população dele emergentes alimentam todo um sistema de transacções particularmente intenso e diversificado entre montante e jusante das populações em mobilidade. Observemos a evolução destes movimentos, na sua pluriformidade, fluxos e(i)migratórios e movimentos turísticos, a part...

  3. Language Awareness in Nova Scotia Schools: An Exploratory Study

    Directory of Open Access Journals (Sweden)

    David Piper

    2010-05-01

    Full Text Available The author conducted a questionnaire survey of language awareness in 358 students studying in Grades 8, 10, and 12 English classes in three rural and three urban schools in Nova Scotia. The main objectives of the study were to learn just how sensitive these students were to key aspects of language prior to any deliberate instruction in language awareness, to obtain new information about levels of natural language awareness as the basis for curriculum development, to uncover significant subject variables in relation to developing language awareness, and to clarify the theoretical distinction between “ordinary” and “critical” language awareness.

  4. Miroljubivi uspon – nova kineska vanjskopolitička teorija

    OpenAIRE

    Baković, Ozren

    2004-01-01

    Kao izraz težnje za osuvremenjivanjem kineske vanjske politike u promijenjenim globalnim uvjetima na početku 21. stoljeća, pojavila se nova službena kineska vanjskopolitička teorija – teorija “miroljubivog uspona”. Nakon što je naviše kinesko rukovodstvo usvojilo teoriju, ona se sad nastoji objasniti međunarodnoj javnosti. Osnovna je postavka teorije “miroljubivog uspona” da snažan dugoročni rast kineskoga gospodarstva i afirmacija Kine u međunarodnim odnosima nije ni regionalna ni globalna p...

  5. Corpos e Corporeidade no Universo da Nova Era no Brasil

    OpenAIRE

    Amurabi Oliveira

    2012-01-01

    O presente trabalho busca explorar a dimensão corpórea enquanto central para a compreensão do fenômeno religioso, em especial do universo Nova Era – NE, em nossa interpretação o corpo apresenta-se enquanto estrutura estruturada estruturante que possibilita aos sujeitos vivenciar e interpretar o mundo, neste sentido, a experiência de imersão e de vivência das práticas da NE são, essencialmente, experiências corpóreas. No decorrer deste trabalho buscaremos dar destaque aos aspect...

  6. CCD Photometry of Dwarf Nova AL Com in Superoutburst

    OpenAIRE

    Pych, W.; Olech, A.

    1995-01-01

    We report a CCD optical photometry of a dwarf nova AL Com in superoutburst. Before superhumps occurred the light curve was highly variable with dominant periods about 41 minutes and 81.5 minutes for different nights. The period of observed superhumps is 82.5 minutes and seems to be stable. The first harmonic of the basic period is also present. We detected a weak signal corresponding to period 78.1 minutes. One of the periods 78.1 or 81.5 is suspected to be a possible signature of orbital mot...

  7. Brief outbursts in the dwarf nova V1316 Cygni

    CERN Document Server

    Shears, J; Poyner, G; Shears, Jeremy; Boyd, David; Poyner, Gary

    2006-01-01

    Several brief outbursts were detected in the dwarf nova V1316 Cyg during 2005. These events have an average amplitude of 1.4 magnitude and a duration of <1 to 2 days. Whilst no outburst period could be confirmed, the shortest period between detected events is 10 days. These curious brief outbursts appear to be the normal pattern of behaviour for this system. They are of smaller amplitude and shorter duration than normal outbursts previously reported in this star. V1316 Cyg appears to be a very unusual system and we suggest that further observations by both amateur and professional astronomers could yield important information about the underlying mechanism.

  8. Guanosina : uma nova abordagem do sistema purinérgico

    OpenAIRE

    Felix Alexandre Antunes Soares

    2005-01-01

    Durante as últimas décadas os estudos do sistema purinérgico concentraram seu foco de atenção nas ações dos derivados da adenina (como adenosina e o ATP). Seus efeitos, receptores, agonistas e antagonistas encontram-se muito bem estabelecidos dentro do sistema nervoso central. Os resultados obtidos com os diversos estudos dos derivados da guanina trazem uma nova perspectiva para o estudo do sistema purinérgico. Os nucleotídeos derivados da guanina são classicamente associados ao sistema de tr...

  9. Novas tecnologias aplicadas às embalagens de alimentos

    OpenAIRE

    Flávia De Floriani Pozza Rebello

    2009-01-01

    Com o desenvolvimento da indústria de alimentos, as embalagens têm se aperfeiçoado, indo além de sua função básica de proteger o alimento contra danos mecânicos e contaminações químicas e microbiológicas. Elas têm cada vez mais desempenhando papel de destaque, contribuindo ativamente para a venda de um produto. Assim, as indústrias de embalagens têm procurado atender aos consumidores mais exigentes e juntamente aos centros de pesquisa e universidades, têm investido mais em estudos de novas te...

  10. Psicofarmacogenética: uma nova abordagem terapêutica

    Directory of Open Access Journals (Sweden)

    Vallada Filho Homero Pinto

    1999-01-01

    Full Text Available A psicofarmacogenética é uma nova área de investigação derivada da psicofarmacologia e da genética. Esta disciplina procura identificar genes de suscetibilidade associados a diferentes padrões de resposta terapêutica e/ou ao variado grau de efeitos colaterais dos psicofármacos. O presente artigo discorrerá, após um breve histórico, sobre alguns exemplos de variantes genéticas relacionadas com a resposta terapêutica de antipsicóticos e antidepressivos.

  11. Orbital period determination in an eclipsing dwarf nova HT Cas

    Science.gov (United States)

    Bąkowska, Karolina; Olech, Arkadiusz

    2014-09-01

    HT Cassiopeiae was discovered over seventy years ago (Hoffmeister 1943). Unfortunately, for 35 years this object did not receive any attention, until the eclipses of HT Cas were observed by Bond. After a first analysis, Patterson (1981) called HT Cas "a Rosetta stone among dwarf novae". Since then, the literature on this star is still growing, reaching several dozens of publications. We present an orbital period determination of HT Cas during the November 2010 super-outburst, but also during a longer time span, to check its stability.

  12. Nova control system: goals, architecture, and system design

    Energy Technology Data Exchange (ETDEWEB)

    Suski, G.J.; Duffy, J.M.; Gritton, D.G.; Holloway, F.W.; Krammen, J.R.; Ozarski, R.G.; Severyn, J.R.; Van Arsdall, P.J.

    1982-05-19

    The control system for the Nova laser must operate reliably in a harsh pulse power environment and satisfy requirements of technical functionality, flexibility, maintainability and operability. It is composed of four fundamental subsystems: Power Conditioning, Alignment, Laser Diagnostics, and Target Diagnostics, together with a fifth, unifying subsystem called Central Controls. The system architecture utilizes a collection of distributed microcomputers, minicomputers, and components interconnected through high speed fiber optic communications systems. The design objectives, development strategy and architecture of the overall control system and each of its four fundamental subsystems are discussed. Specific hardware and software developments in several areas are also covered.

  13. A nova alfabetização por (em) computador

    OpenAIRE

    Reinking, David

    2013-01-01

    Neste artigo o autor apresenta argumentos para ampliar os conceitos de alfabetização no intuito de dar espaço para a escrita e a leitura de textos eletrônicos. Relaciona quatro características dos texto eletrônicos que subjazem à nova alfabetização por(em) computador. Os textos eletrônicos (a) facilitam uma interação entre leitores e textos. (b) podem influenciar a leitura pelo fato de limitar o acesso ao texto, (c) podem apresentar uma estrutura diferente do que os textos impressos, e (d) em...

  14. O Transito e o Turismo na Cidade de caldas Novas - GO / TRAFFIC AND TOURISM IN THE CALDAS NOVAS CITY - BRAZIL

    Directory of Open Access Journals (Sweden)

    Norma Urban Gomes

    2010-05-01

    Full Text Available Resumo: Este trabalho tem como objetivo, mostrar a relação intrínseca entre o trânsito e o turismo na cidade de Caldas Novas – GO. Deste modo, para estudarmos o trânsito e seus elementos, bem como todos os fatores positivos e negativos do mesmo na cidade teremos necessariamente que falar a respeito do turismo, pois é partir dessa premissa que se molda a questão da Geografia dos Transportes em Caldas Novas,cidade esta que se destaca pelo apelo turístico de suas águas termais. A Geografia se preocupa com o inter-relacionamento ambiental e humano em um contexto espacial, e Geografia dos Transportes é o estudo dos sistemas de transportes e seus impactos espaciais. Os meios de transporte são essenciais em uma cidade turística, pois o fluxo de pessoas, bens e serviços dependem substancialmente da condição de circulação. Esse trabalho justifica-se pela necessidade de compreender e avaliar a situação do trânsito na cidade de Caldas Novas nos períodos de alta temporada, quando a cidade sofre intensa movimentação turística,causando um grande acumulo de veículos e pessoas nas vias de circulação. Isso dificulta além obviamente da circulação das pessoas como a circulação de bens e serviços essenciais para que a atividade turística se desenvolva satisfatoriamente. O estudo dos transportes é, sobretudo, multidisciplinar por natureza, e algumas vezes também interdisciplinar.

  15. Library Cooperation at the NOVA University--the Nordic University in Agriculture, Forestry and Veterinary Medicine.

    Science.gov (United States)

    Myllys, Heli

    The Nordic University in Agriculture, Forestry and Veterinary Medicine--the NOVA University-was established in 1995 to increase the cooperation between the Nordic agricultural universities. The NOVA libraries of the seven institutions and facilities involved wanted to show that they are a very useful partner in launching new ideas. They have the…

  16. A Light Curve Analysis of Classical Novae: Free-free Emission vs. Photospheric Emission

    CERN Document Server

    Hachisu, Izumi

    2014-01-01

    We analyzed light curves of seven relatively slower novae, PW Vul, V705 Cas, GQ Mus, RR Pic, V5558 Sgr, HR Del, and V723 Cas, based on an optically thick wind theory of nova outbursts. For fast novae, free-free emission dominates the spectrum in optical bands rather than photospheric emission and nova optical light curves follow the universal decline law. Faster novae blow stronger winds with larger mass loss rates. Since the brightness of free-free emission depends directly on the wind mass loss rate, faster novae show brighter optical maxima. In slower novae, however, we must take into account photospheric emission because of their lower wind mass loss rates. We calculated three model light curves of free-free emission, photospheric emission, and the sum of them for various WD masses with various chemical compositions of their envelopes, and fitted reasonably with observational data of optical, near-IR (NIR), and UV bands. From light curve fittings of the seven novae, we estimated their absolute magnitudes,...

  17. Novas Cartas Portuguesas: The Making of a Reputation

    Directory of Open Access Journals (Sweden)

    Ana Margarida Dias Martins

    2012-05-01

    Full Text Available Novas Cartas Portuguesas (New Portuguese Letters, co-authored by Maria Isabel Barreno, Maria Teresa Horta, and Maria Velho da Costa, was banned in 1972 in Portugal for exploring sensitive issues such as women's oppression under the Catholic patriarchy. Given that police action against the authors soon became the focus of an international feminist protest in 1972-73, existing discussions of the book's reception often focus almost exclusively on what may be called its political life. I propose to approach the book from a new angle, with the purpose of uncovering its theoretical dimension as a literary-critical text that may have played an important role in helping to shape feminist intellectual directions of the 1970s. Specifically, I analyze how a general insistence on the political life of Novas Cartas contributed to marginalizing the work on a theoretical level, transforming it into a "strange" (Ahmed textual body out of place. In a manner similar to what would later happen to the Brazilian writer Clarice Lispector as a result of Hélène Cixous's feminist sponsorship of her work, this marginalization helped define the boundaries of "international feminism" as opposed to "Portuguese anti-fascism," according to a conception of the Lusophone cultural sphere as an anachronistic feminine space for political action, entirely disconnected from the centers where feminist theory is made.

  18. The unusual Nova Cygni 2006 (V2362 Cyg)

    CERN Document Server

    Kimeswenger, S; Knapp, A; Schafer, J; Unterguggenberger, S; Weiss, S

    2008-01-01

    Context: Optical nova lightcurves often have structures, such as rapid declines and recoveries, due to nebular or dusty phases of the ejecta. Nova Cygni 2006 (V2362 Cyg) underwent an unusual brightening after an early rapid decline. The shape of the lightcurve can be compared to that of V1493 Aql, but the whole event in that case was not as bright and only lasted a couple of weeks. V2362 Cyg had a moderately fast decline of t_2 = 9.0 before rebrightening, which lasted 250 days after maximum. Aims: We present an analysis of our own spectroscopic investigations in combination with AAVSO photometric data covering the whole rebrightening phase until the return to the final decline. Methods: We used the medium resolution spectroscopy obtained in ten nights over a period of 79 nights to investigate the change of the velocity structure of the ejecta. The publicly available AAVSO photometry was used to analyze the overall properties and the energy of the brightening. Results: Although the behavior of the main outburs...

  19. Mixing in classical novae: a 2-D sensitivity study

    CERN Document Server

    Casanova, Jordi; Garcia-Berro, Enrique; Calder, Alan; Shore, Steven N

    2010-01-01

    Classical novae are explosive phenomena that take place in stellar binary systems. They are powered by mass transfer from a low-mass, main sequence star onto a white dwarf. The material piles up under degenerate conditions and a thermonuclear runaway ensues. The energy released by the suite of nuclear processes operating at the envelope heats the material up to peak temperatures of ~ (1 - 4) \\times 108 K. During these events, about 10-4 - 10-5 M\\odot, enriched in CNO and other intermediate-mass elements, are ejected into the interstellar medium. To account for the gross observational properties of classical novae (in particular, a metallicity enhancement in the ejecta above solar values), numerical models assume mixing between the (solar-like) material transferred from the companion and the outermost layers (CO- or ONe-rich) of the underlying white dwarf. The nature of the mixing mechanism that operates at the core-envelope interface has puzzled stellar modelers for about 40 years. Here we investigate the rol...

  20. The formation of Cataclysmic Variables: the influence of nova eruptions

    CERN Document Server

    Nelemans, G; Repetto, S; Toonen, S; Phinney, E S

    2015-01-01

    The theoretical and observed populations of pre-cataclysmic variables (pre-CVs) are dominated by systems with low-mass white dwarfs (WDs), while the WD masses in CVs are typically high. In addition, the space density of CVs is found to be significantly lower than theoretical models. We investigate the influence of nova outbursts on the formation and (initial) evolution of CVs. In particular, we calculate the stability of the mass transfer in case all the material accreted on the WD is lost in classical novae, and part of the energy to eject the material comes from a common-envelope like interaction with the companion. In addition, we study the effect of an asymmetry in the mass ejection, that may lead to small eccentricities in the orbit. We find that a common-envelope like ejection significantly decreases the stability of the mass transfer, in particular for low-mass WD. Similarly, the influence of asymmetric mass loss can be important for short-period systems and even more so for low-mass WD, but likely dis...

  1. IX Draconis - a curious ER UMa-type dwarf nova

    CERN Document Server

    Otulakowska-Hypka, M; de Miguel, E; Rutkowski, A; Koff, R; B\\kakowska, K

    2012-01-01

    We report results of an extensive world-wide observing campaign devoted to a very active dwarf nova star - IX Draconis. We investigated photometric behaviour of the system to derive its basic outburst properties and understand peculiarities of IX Dra as well as other active cataclysmic variables, in particular dwarf novae of the ER Uma-type. In order to measure fundamental parameters of the system, we carried out analyses of the light curve, O-C diagram, and power spectra. During over two months of observations we detected two superoutbursts and several normal outbursts. The V magnitude of the star varied in the range 14.6 - 18.2 mag. Superoutbursts occur regularly with the supercycle length of 58.5+/-0.5 d. When analysing data over the past 20 years, we found that the supercycle length is increasing at a rate of P_dot = 1.8 * 10^{-3}. Normal outbursts appear to be irregular, with typical occurrence times in the range 3.1 - 4.1 d. We detected a double-peaked structure of superhumps during superoutburst, with ...

  2. A remarkable recurrent nova in M31 - The optical observations

    CERN Document Server

    Darnley, M J; Bode, M F; Henze, M; Ness, J -U; Shafter, A W; Hornoch, K; Votruba, V

    2014-01-01

    Context. In late November 2013 a fourth outburst in five years of the M31 recurrent nova M31N 2008-12a was announced. Aims. In this Letter we address the optical lightcurve and progenitor system of M31N 2008-12a. Methods. Optical imaging data of the 2013 outburst from the Liverpool Telescope, La Palma, and Danish 1.54m Telescope, La Silla, and archival Hubble Space Telescope near-IR, optical and near-UV data are astrometrically and photometrically analysed. Results. Photometry of the 2013 outburst, combined with the previous three, enabled construction of a template lightcurve of a very fast nova (t2 (V) ~4 days). The archival data allowed recovery of the progenitor system in optical and near-UV data, indicating a red-giant secondary with bright accretion disk, or alternatively a system with a sub-giant secondary but dominated by a disk. Conclusions. The outbursts of M31N 2008-12a, plus a number of historic X-ray detections, indicate a unique system with a recurrence timescale of ~1 year. This implies the pre...

  3. The NOvA νe Appearance Analysis

    Science.gov (United States)

    Colo, Marco; NOvA Collaboration

    2017-01-01

    Since neutrino oscillations were first detected, oscillation experiments have managed to measure most of the parameters that govern this phenomenon. Major unknowns remain: the mass ordering - whether ν3 is the heaviest neutrino state, or the lightest; CP Violation - whether neutrino oscillation violate CP symmetry, and, if so, how big is the CP-violating phase δCP; and, the θ23 octant - whether the value of θ23 resides in the lower octant (θ23 45°) or is exactly maximal (θ23 =45°). NOvA, with its 810 km baseline, the longest of any currently running experiment, and its capability to switch between a νμ source and a νμ source, is extremely well positioned to address these questions. In this talk, I will discuss the νe appearance analysis in NOvA: I will illustrate the analysis method, discuss the results that we have obtained in the latest round of analysis, and talk about what we expect from future runs.

  4. A study of the shell of Nova V2659 Cyg

    Science.gov (United States)

    Tarasova, T. N.

    2016-12-01

    Results of a study of the shell of Nova V2659 Cyg based on spectrophotometric observations carried out over a year and a half after its eruption are presented. The physical conditions in the nova shell have been studied. The electron temperature (9000 K) and density (5 × 106 cm-3) in the nebular stage have been estimated, together with the abundances of helium, oxygen, nitrogen, neon, argon, and iron. The abundances of nitrogen, oxygen, neon, and argon are enhanced relative to the solar values. The relative abundances are [N/H] = 2.26 ± 0.25 dex, [O/H] = 1.66 ± 0.35 dex, [Ne/H] = 0.78 ± 0.25 dex, and [Ar/H] = 0.32 ± 0.38 dex. The estimated mass of oxygen and total mass of the emitting shell are ≈1 × 10-4 M ⊙ and ≈3 × 10-4 M ⊙, respectively. In the period of chaotic brightness oscillations, the maximum velocity of the shell expansion derived from the radial velocities of the absorption components of the HI and FeII line profiles increased by ≈400 km/s 41 days after the maximum, and by ≈200 km/s 101 days after the maximum, reaching 1600 km/s in both cases.

  5. Optical spectroscopy of the dwarf nova U Geminorum

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    Morales-Rueda, T R

    2006-01-01

    U Gem is unique in having a direct measurement of K1 = 107 +- 2 km/s, Long et al. 1999). We present high-resolution optical spectra of the dwarf nova U Gem in quiescence taken to test the accuracy to which the HST value can be recovered from optical data. We find that, even with data of very high S/N we cannot recover Long et al.'s value to better than about 20% by any method. Contamination by neighbouring emission lines seems a likely culprit. Our data reveal a number of new features: Doppler tomograms show emission at low velocity, close to the centre of mass, and a transient, narrow absorption feature is seen in the Balmer lines near the line centres at the time of eclipse. We suggest that stellar prominences, as previously invoked for the dwarf novae IP Peg and SS Cyg in outburst, may explain both of these features. The He II 4686.75 A line emission is dominated by the gas stream/disc impact region. Two distinct spots are seen in Doppler maps, the first being very narrow and showing a velocity close to th...

  6. Pan-chromatic observations of the remarkable nova LMC 2012

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    Schwarz, Greg J; Page, Kim L; Osborne, Julian P; Beardmore, Andrew P; Walter, Frederick M; Bode, Michael F; Drake, Jeremy J; Ness, Jan-Uwe; Starrfield, Sumner; Van Rossum, Daniel R; Woodward, Charles E

    2014-01-01

    We present the results of an intensive multiwavelength campaign on nova LMC 2012. This nova evolved very rapidly in all observed wavelengths. The time to fall two magnitudes in the V band was only 2 days. In X-rays the super soft phase began 13$\\pm$5 days after discovery and ended around day 50 after discovery. During the super soft phase, the \\Swift/XRT and \\Chandra\\ spectra were consistent with the underlying white dwarf being very hot, $\\sim$ 1 MK, and luminous, $\\sim$ 10$^{38}$ erg s$^{-1}$. The UV, optical, and near-IR photometry showed a periodic variation after the initial and rapid fading had ended. Timing analysis revealed a consistent 19.24$\\pm$0.03 hr period in all UV, optical, and near-IR bands with amplitudes of $\\sim$ 0.3 magnitudes which we associate with the orbital period of the central binary. No periods were detected in the corresponding X-ray data sets. A moderately high inclination system, $i$ = 60$\\pm$10$^{\\arcdeg}$, was inferred from the early optical emission lines. The {\\it HST}/STIS ...

  7. Guerra do Golfo: a crise da nova ordem mundial

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    Virgílio Caixeta Arraes

    2004-06-01

    Full Text Available Este artigo, tomando como ponto de partida as Guerras do Golfo, traça o perfil da nova ordem mundial formada com a derrocada da União Soviética e o fim da Guerra Fria, e a ascensão dos Estados Unidos como única superpotência no século XXI. O autor também afirma que a nova ordem mundial, proclamada com vistas à promoção permanente do desenvolvimento e da paz, residiria no binômio político-econômico da democracia neoliberal.This article, taking as a starting point the Gulf Wars, traces the profile of the new world order that took shape with the end of Cold War and the Soviet Union, and the raise of the United States as the major power in the 21st century. The author also affirms that the new world order, proclaimed in order to promote permanent development and peace, combines the economic-politic binomial of the neo-liberal democracy.

  8. Uma nova cidade para as águas urbanas

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    Renato Luiz Sobral Anelli

    2015-08-01

    Full Text Available O artigo apresenta os paradigmas que podem ser revistos para que no futuro não se repita a grave crise de abastecimento de água nas grandes regiões metropolitanas da macrometrópole paulista. Inicia por um breve histórico do desenvolvimento urbano da Região Metropolitana de São Paulo e sua relação com os recursos hídricos, destacando os planos e projetos que servem de exemplos para uma nova concepção urbanística para as águas urbanas. Destaca as oportunidades abertas pela revisão do aparato de ordenação urbana de São Paulo, iniciada pelo novo Plano Diretor Estratégico, no qual estão propostos instrumentos de planejamento e gestão capazes de amparar uma nova forma de cidade para as águas urbanas.

  9. The astronomizings of Dr. Anderson and the curious case of his disappearing nova

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    Shears, Jeremy

    2012-01-01

    Dr. Thomas David Anderson (1853-1932) was a Scottish amateur astronomer famed for his discovery of two bright novae: Nova Aurigae 1891 and Nova Persei 1901. He also discovered more than 50 variable stars as well as making independent discoveries of Nova Aquilae 1918 and comet 17P/Holmes in 1892. At the age of seventy, in 1923, he reported his discovery of a further nova, this time in Cygnus. This was set to be the culmination of a lifetime devoted to scanning the night sky, but unfortunately no one was able to confirm it. This paper discusses Anderson's life leading up to the discovery and considers whether it was real or illusory.

  10. Perfil dos ácidos graxos da carcaça de cordeiros alimentados com grãos de canola em diferentes formas Meat fatty acid profile of lambs fed processed or unprocessed canola seeds

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    Francisco de Assis fonseca de Macedo

    1999-11-01

    Full Text Available O objetivo deste trabalho foi determinar a alteração do perfil dos ácidos graxos da carcaça de ovinos alimentados com dietas contendo grãos inteiros de canola (CI em duas formas de processamentos (quebrados - CQ ou peletizados - CP. Foram utilizados 28 cordeiros, distribuídos num delineamento inteiramente casualizado e abatidos com média de peso vivo entre 31 e 33kg, coletando-se amostras entre a 12ª e 13ª costela. Houve diferença significativa para os ácidos graxos C10:0, C14:1ω5, C15:0, C16:0, C16:1ω7e C17:0, cujas médias foram maiores que na dieta controle. Os ácidos graxos C18:0, C18:1ω9, C18:3ω6, C18:3ω3, C20:0, C20:1ω9, C22:0 e C24:0 sofreram alterações com a inclusão de grãos de canola. Também foi observado diferença significativa para os totais de ácidos graxos mono-insaturados, porém, os totais de ácidos graxos polinsaturados e a relação entre ácidos graxos polinsaturados e saturados foram inalterados. Os resultados levam à conclusão de que a inclusão de grãos inteiros de canola nas dietas para cordeiros altera o perfil dos ácidos graxos independentemente da forma de apresentação.The objective of this experiment was to compare carcass fatty acids profile of lambs fed a control diet and diets containing either whole (WC, cracked (CC or pelleted (PC canola seeds. Twenty-eight lambs assigned to a completely randomized design were fed their respective diets for 132 days and slaughtered between 31 and 33kg of body weight. Samples of muscle Longissimus dorsi, Psoas maior and Psoas menor were collected on the left side of the carcass between the 12th and 13th ribs and 11 cm from the carcass midline. Concentrations of C10:0, C14:ω5, C15:0, C16:0, C16:1ω7. C17:0 and, C18:3ω3 were significantly higher (P < 0.05 in the carcass of lambs fed the three canola seed diets than in the carcass of those fed the control diet. Pelleted canola seeds increased the percentages of C18:1ω9, C18:3ω6, C20:0, C20:1ω9, C22

  11. Performance of lambs weaned at 67 days of age and fed corn silage and oat hay/ Desempenho de cordeiros desmamados aos 67 dias alimentados com silagem de milho e feno de aveia

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    Adriana Pereira da Silva

    2003-05-01

    Full Text Available This work had as objectives to evaluate the performance of lambs weaned at 67 days of age and fed with different roughage sources in confinement. Thirty animals out of Corriedale ewes mated to Hampshire Down, Ile de France and Suffolk rams, were used. After weaning the animals were fedlot and distributed in one of the following treatments: T1 – Corn silage + concentrate; T2 – Corn silage and oat hay (50% each + concentrate; and T3 – Oat hay + concentrate. It was used a 60:40 roughage:concentrate ratio, dry matter basis. At the beginning of the experiment the animals weighed 11.51, 12.46 and 12.33 kg (P>0.05, and after nine weeks of feedlot the weights were 17.53, 19.34 and 19.35 kg (P>0.05, respectively, for T1, T2 e T3. Average daily weight gain was similar (P>0.05 among treatments. It was not observed differences (P>0.05 in weights and weight gains among the genetic groups. However, male lambs presented greater average daily weight gain than female lambs (0.120 x 0.091 kg. There were no differences in feed conversion among the treatments, however, animals from the T2 had greater dry matter intake. It can be concluded that either corn silage or oat hay can be used for feeding weaned lambs.Este trabalho teve como objetivo avaliar o desempenho de cordeiros desmamados aos 67 dias e alimentados com diferentes fontes de volumosos em confinamento. Foram utilizados 30 animais oriundos de cruzamentos entre ovelhas Corriedale e carneiros Hampshire Down, Ile de France e Suffolk. Logo após o desmame os animais foram confinados, sendo distribuídos para receberem um dos tratamentos: T1 – Silagem de milho mais concentrado; T2 – Silagem de milho e feno de aveia (50% do volumoso cada mais concentrado; e T3 – Feno de aveia mais concentrado. A proporção volumoso:concentrado utilizada foi de 60:40, base seca. Os pesos médios dos animais no início do experimento foram de 11,51; 12,46 e 12,33 kg (P>0,05 e os pesos finais, após nove semanas de

  12. Dextran iron in anemic lambs: effects on reticulocytosis and free radical production Ferro dextrano em cordeiros anêmicos: efeitos na reticulocitose e produção de radicais livres

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    Ricardo Xavier da Rocha

    2007-10-01

    Full Text Available Anemia due to worm infection is a major cause of loss in the sheep industry, due to deaths, drop in average daily gains and long recovery time following treatment. The present experiment was aimed at evaluating the oxidative status and the recovery of red blood cell (RBC profile in lambs with induced anemia by bleeding, treated or not with dextran iron. Ten ram lambs 5 to 7 months old were used. Blood samples were drawn every other day and when reached packed cell volume (PCV of 15% were randomly allocated (day zero to one of the experimental groups. Treated group received a single dose of 25mg per kg body weight of a commercial formulation of dextran iron, the control group received no treatment. Blood samples were taken on days 0, 7, 14, and 21 after treatment. On days 7 an 21 treated animals presented higher thyobarbituric acid reactive species (TBARS values, reduced non-protein thiol groups (NPTH levels were found in the treated group on days 7, 14 and 21. Erythrocyte membrane resistance to osmotic challenge was improved on day 7 in treated animals. Recovery to normal values for the RBC profile was faster in the treated group with significant differences starting on day 7. It was conclude that althouth the iron treatment increased the oxidative stress, it also accelerated recovery of the hematological profile. Moreover, it did not increase hemolysis in anemic blood by the action of oxygen reactive species upon biological membranes.A anemia verminótica é a principal causa de perdas na ovinocultura, incluindo diminuição no ganho médio diário, demora no tempo de recuperação pós-tratamento e óbito. O objetivo deste trabalho foi avaliar o status oxidativo e a recuperação do quadro hematológico de cordeiros com anemia induzida por flebotomia e suplementados ou não com ferro dextrano. Foram utilizados dez cordeiros machos entre cinco e sete meses de idade. O dia zero do experimento foi considerado quando cada animal atingiu o hemat

  13. Características sensoriais da carne de cordeiros da raça Santa Inês submetidos a diferentes dietas Sensory characteristics of meat of Santa Inês lamb submitted to different diets

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    Sibelli Passini Barbosa Ferrão

    2009-02-01

    Full Text Available As características sensoriais da carne, como sabor e aroma, podem ser influenciadas por diversos fatores, sendo que a alimentação é considerada o de maior importância. Objetivou-se avaliar o efeito de diferentes dietas sobre as propriedades sensoriais da carne de cordeiros, três dietas à base de silagem de cana-de-açúcar e polpa de citrus, em diferentes relações concentrado: volumoso (100:0; 75:25; 50:50, foram fornecidas a 21 cordeiros, machos, da raça Santa Inês, que foram abatidos aos 35kg, com idade média de 199 dias. Após o abate, as carcaças foram mantidas resfriadas a -2ºC/24h e em seguida retirado o músculo Longissimus dorsi (LD, para a análise sensorial. As amostras cozidas foram servidas a um painel de 12 provadores treinados para avaliação sensorial dos atributos de aparência, sabor, aroma, maciez e suculência. A avaliação realizada pelos provadores demonstrou que não houve efeito significativo (P>0,05 da dieta sobre os atributos de sabor, maciez e suculência. Entretanto, a aparência e o aroma sofreram influência, com diferença significativa entre os tratamentos 100:0 e 50:50. O aroma mais forte a "ovino" e a aparência mais "desagradável" foram mais evidentes nos animais alimentados com a dieta 100:0. As amostras provenientes dos animais alimentados com a dieta 50:50 apresentaram-se de melhor qualidade sensorial em relação às demais dietas.The sensory characteristics of meat, such as flavor and aroma, may be influenced by several factors, and the use as food is considered the most important. With the aim of evaluating the effects of different diets on the sensorial properties of the meat of lambs, three diets having sugar cane ensilage and pulp of citrus as a base, differing only in the proportion of concentrated: forage (100:0; 75:25; 50:50, were offered to 21 lambs of Santa Inês breed, that were slaughtered with 35 kg, with an average age of 199 days. After slaughter, the carcasses were kept

  14. Parasitological characteristics and tissue response in the abomasum of sheep infected with Haemonchus spp. Características parasitológicas e resposta tissular do abomaso em cordeiros infectados por Haemonchus spp.

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    T.C.G. Oliveira-Sequeira

    2000-10-01

    Full Text Available A histopathological study was conducted on the abomasal mucosa of 40 Corriedale sheep exposed to natural infection with Haemonchus spp. The sheep were allowed to graze on contaminated pastures for 14 days and, after being housed for 28 days, they were slaughtered. Fecal samples were collected for fecal egg counts (FEC and abomasum samples were obtained for histopathological examination and eosinophil, mast cell and globule leucocyte counts. The number of Haemonchus spp. present in the abomasum was estimated from a 10% aliquot of its content. The number of eggs per female was estimated for 10 Haemonchus spp. females collected from each animal. The following significant correlation coefficients were obtained between the characteristics analyzed: number of Haemonchus and FEC (r = 0.86, female length and number of eggs per female (r = 0.60, female length and FEC (r = 0.53, number of eosinophils and number of Haemonchus (r = 0.48, number of eosinophils and number of globule leucocytes (r = 0.54, number of mast cells and female length (r = -0.39, and number of mast cells and number of globule leucocyte (r = 0.34. The characteristics that showed the highest correlation with animal load was FEC.Realizou-se um estudo histopatológico da mucosa do abomaso de 40 cordeiros da raça Corriedale, expostos à infecção natural por Haemonchus spp. Os cordeiros foram colocados em pastagens contaminadas por 14 dias e após 28 dias de estabulação foram necropsiados. Por ocasião da necropsia, foram colhidas amostras de fezes para a realização da contagem de ovos por grama de fezes (OPG e amostras do abomaso para exame histopatológico e contagem do número de eosinófilos, mastócitos e leucócitos globulares. O número de Haemonchus spp. presente no abomaso foi estimado a partir de uma alíquota de 10% do conteúdo. O número de ovos por fêmea foi estimado em 10 fêmeas de Haemonchus spp. colhidas de cada animal. Coeficientes de correlação significativos

  15. Crescimento de cordeiros abatidos com diferentes pesos: osso, músculo e gordura da carcaça e de seus cortes Growth of lambs slaughtered at different weights: bone, muscle and fat of the carcass and its cuts

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    Lisiane Furtado da Silva

    2000-08-01

    Full Text Available O trabalho foi realizado no Setor de Ovinocultura do Departamento de Zootecnia da Universidade Federal de Santa Maria, objetivando determinar as quantidades de osso, músculo e gordura da carcaça e o crescimento de osso e músculo da carcaça e dos diferentes cortes da mesma. Foram utilizados 22 cordeiros machos inteiros, filhos de carneiros Texel e ovelhas cruza (Texel x Ideal. Desses, quatro/oram abatidos no início do experimento (24 horas após o nascimento, e os restantes, ao desmame (45 dias de idade e aos 28 e 33kg. Os cordeiros foram confinados em baias individuais, com suas respectivas mães, até o desmame (45 dias de idade. A determinação do crescimento dos tecidos da carcaça e de seus cortes (quarto, paleta, costela, espinhaço e pescoço foi realizada através de equações alométricas, utilizando-se o logaritmo do peso de osso ou músculo, em função do logaritmo do peso de corpo vazio (PCV ou peso de carcaça fria (PCF. As quantidades de osso e músculo aumentaram (P0,05 com a elevação do peso de carcaça fria. A proporção de gordura aumentou do nascimento ao desmame (PThis experiment was developed at the Ovine Section of Animal Science Department, at Federal University of Santa Maria, Brazil- The purpose of this experiment was to determine the quantity of bone, muscle and fat of the carcass, and the growth ofbone and muscle of the carcass, and of the carcass cuts. Twenty-two intact mate lambs, sired by Texel males, from crossbreed Texel -Ideal dams were used. Four lambs were siaughtered at the beginning of the experiment (24 hours after birth and groups of six lambs were siaughtered at weaning and when reaching 28 and 33kg. The lambs were kept in individual stalls together with their respective mothers until weaning (45 days of age. To study the growth of the carcass tissues and carcass cuts (hindquarter, shoulder, rib, backbone, neck, regression equations of the log of weight of each tissue, as a function of the log of

  16. Características físico-químicas e sensoriais da carne de cordeiros de diferentes genótipos terminados em confinamento Physicochemical and sensory attributes of lamb meat from different genotypes feedlot finished

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    Ângela Maria de Vasconcelos

    2011-03-01

    Full Text Available Avaliou-se com este estudo a influência de diferentes genótipos sobre a composição centesimal, perda de peso por cocção e qualidade sensorial da carne de cordeiros meio sangue obtidos por cruzas entre animais Sem Padrão Racial Definido com Dorper, Santa Inês e Somalis terminados em confinamento no semiárido nordestino. Foram avaliadas amostras provenientes de 24 animais, oito de cada genótipo. A dieta foi constituída de milho, farelo de trigo, farelo e óleo de soja e continha 2,8Mcal de EM/kg de MS para todos os animais. Os animais foram desmamados entre 70 e 84 dias. A terminação durou 90 dias, quando foram abatidos e as carcaças mantidas em uma câmara frigorífica a 4°C, por 24 horas. Após esse período, foram seccionados os músculos Longissimus dorsi, embalados a vácuo, identificados e armazenados a -20°C para análises da composição centesimal, perda de peso por cocção e avaliação das características sensoriais. Não foi observada diferença nos percentuais de proteínas, lipídios, cinzas e nos parâmetros suculência, aroma e sabor. Em contrapartida, o teor de umidade, a perda de peso por cocção, a dureza e aceitação global apresentaram diferenças estatísticas entre os grupos, o que evidencia a influência do genótipo sobre os atributos da carne de cordeiros, e isto confere ao produto características sensoriais diferenciadas.The aim of this study was to evaluate the influence of different genotypes on the proximate composition, weight loss due to cooking, and sensory quality of lamb meat from half-blooded lambs obtained by crosses between undefined breed animals with Dorper, Santa Inês and Somalis feedlot finished in the northeastern semiarid region of Brazil. Samples from 24 animals were evaluated, eight from each genotype. The diet consisted of corn, wheat bran, soybean bran and oil, containing 2.8Mcal EM/kg of DM for all animals. The animals were weaned between 70 and 84 days of age. The termination

  17. CHARACTERIZATION OF RUMINAL AND METABOLIC PARAMETERS IN CAMBS RAISED IN NATIVE PASTURE CARACTERIZAÇÃO DOS PARÂMETROS RUMINAIS E METABÓLICOS DE CORDEIROS MANTIDOS EM PASTAGEM NATIVA

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    Felix Hilário Diaz González

    2007-12-01

    Full Text Available

    The objective was aimed at with this work to charac-terize the parameters in ruminal and metabolic parameters in weaned lambs kept in native pasture. Ten lambs were used – five males and five females – with average body weights medium of  26 kg and 22.5 kg, respectively, and ages between 75 and 95 days old. Lambs were weaned and permanently kept in native pasture. Samples of ruminal fluid were collected during eight weeks, and nine collects. Oxidation-reduction, time of sedimentation-flotation, pH, color, odor, viscosity and motility of protozoa were evaluated. Blood samples were also collected to determine metabolic profiles through concentrations of glucose, triacylglycerids, cholesterol, urea, albumin, aspartate amino transferase and γ-glutamil transferase. Ruminal parameters did not differ between gender at α = .05 except for pH which was higher (P < .05 in females (6.90 than in males (6.80. A similar result was observed in the metabolic parameters, with no statistically significant difference between genders at α = .05. However, albumin concentration was higher on males (2.10mg/dL than in females (2.02mg/dL. The results suggest that males and females have similar ruminal and metabolic profiles except for a higher pH in females and a higher albumin concentration in males.

    Key-words: Metabolism, sheep, native pastura, rumen.

    Objetivou-se com este trabalho caracterizar os parâmetros ruminais e metabólicos de cordeiros machos e fêmeas, os quais foram mantidos em pastagem nativa. Utilizaram-se dez cordeiros, sendo cinco machos e cinco fêmeas, com peso médio ao desmame de 26 ±5,43 e 22,5 ± 4,06 kg, respectivamente, com idades entre 75 e 95 dias. Após o desmame, os animais foram mantidos permanentemente em pastagem nativa, por um período de oito semanas. Efetuaram-se nove coletas de amostras de fluido rumina, para determina

  18. Desempenho e digestibilidade in vivo de cordeiros alimentados com dietas contendo canola em grão integral em diferentes formas Performance and digestibility in vivo of lambs fed diets with whole canola grain in different forms

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    Vanderlei Bett

    1999-08-01

    Full Text Available O desempenho e a digestibilidade dos nutrientes de cordeiros alimentados com concentrados formulados com farelo de soja (FS, canola integral (CI canola quebrada (CQ ou canola peletizada (CP e feno de aveia, fornecidos na relação 30/70 (volumoso/conconcentrado, %MS foram avaliados. Vinte oito cordeiros machos com idade inicial entre 60 e 90 dias e 17 kg PV foram distribuídos em delineamento inteiramente casualizado. As ingestões (g/d de MS, PB, FDA, FDN e EB (Mcal/dia, o ganho médio diário e a conversão alimentar, foram semelhantes. Não houve diferenças para digestibilidade aparente da MS, PB e EB, exceto para digestibilidade de FDN (46,84; 60,11; 50,10; e 38,88% e FDA (45,84; 54,19; 46,57; e 29,59% para FS, CI, CQ e CP, respectivamente. Houve menor retenção de nitrogênio para CP (3,0 g/d em comparação às outras dietas (entre 5,0 e 7,3 g/d. Os tratamentos não diferiram na concentração de propionato, mas reduziram as concentrações de butirato (7,08; 4,87; 4,08; e 4,29 μM/mL de líquido ruminal e N-amoniacal (12,17; 8,69; 8,40; e 7,66 mg/100 mL de líquido de rúmen. O uso de canola, nas diferentes formas, não influenciou a ingestão e a digestão, proporcionando desempenho semelhante entre os tratamentos.The performance and digestibility of nutrients of lambs fed concentrates formulated with soybean meal (SM and whole canola grain (WC, cracked canola grain (CC or pelleted canola (PC and oat hay, fed in a 30:70 (forage to concentrate ratio, %DM were evaluated. Twenty-eight male lambs with initial age from 60 to 90 days and 17 kg LW were allotted to a completely randomized design. The intakes (g/d of DM, CP, ADF, NDF and GE (Mcal/d, the average daily gain and feed: gain ratio, were similar. There were no differences for apparent digestibilities of MS, PB and GE, except for the NDF digestibility (46.84, 60.11, 50.10, and 38.88% and ADF (45.84, 54.19, 46.57, and 29.59% for SM, WC, CC and PC, respectively. There was lower nitrogen

  19. Eficiência bioeconômica de cordeiros F1 Dorper x Santa Inês para produção de carne Bioeconomic efficiency of F1 Dorper x Santa Inês lambs for meet production

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    Nelson Nogueira Barros

    2005-08-01

    Full Text Available O objetivo deste trabalho foi avaliar a eficiência bioeconômica de cordeiros F1 Dorper x Santa Inês para produção de carne. Analisou-se o desempenho de ovinos ½ sangue Dorper x ½ sangue Santa Inês, nas fases de cria e de acabamento. A fase de produção das crias foi realizada em caatinga nativa e a fase de acabamento em confinamento. As matrizes foram suplementadas nos últimos 50 dias de prenhez e nos primeiros 30 dias de lactação. As crias foram desmamadas aos 70 dias de idade, divididas em três lotes e confinadas, alimentadas com capim-elefante (Pennisetum purpureum ad libitum e concentrado na proporção de 1,5%, 2,5% e 3,5% do peso vivo, respectivamente. O sexo não exerceu influência sobre os pesos no nascimento, no desmame, nem sobre o ganho em peso até o desmame. Não foi observada influência do sexo sobre os pesos e os ganhos em peso aos 30 e 50 dias de confinamento. Nas fases de produção e acabamento em confinamento, os animais de nascimento simples foram superiores aos de nascimento duplo quanto a essas variáveis. Houve efeito linear significativo para peso e ganho em peso aos 30 e 50 dias de confinamento. Os três níveis de uso de concentrado foram economicamente viáveis. As margens brutas de peso vivo, por kg de cordeiro produzido, foram de R$ 0,26 kg-1, R$ 0,30 kg-1 e R$ 0,36 kg-1 para concentrados a 1,5%, 2,5% e 3,5% do peso vivo, respectivamente. Os melhores resultados econômicos foram obtidos quando o nível de concentrado foi de 3,5% do peso vivo.The objective of this work was to evaluate bioeconomic efficiency of F1 Dorper x Santa Inês lambs for meet production. Performance of F1 Dorper x Santa Inês lambs in raising and fattening phases was analyzed. The production phase of lambs was realized in native pastures ("caatinga" and the finishing phase was in confinement. The ewes were supplemented during the last 50 days of pregnancy and the first 30 days of lactation. Lambs were weaned at 70 days of age

  20. Comportamento ingestivo de cordeiros alimentados com dietas contendo diferentes níveis de fibra em detergente neutro Ingestive behavior of lambs fed with a diet of different levels of fiber in neutrol detergent

    Directory of Open Access Journals (Sweden)

    Adriano Ramos Cardoso

    2006-04-01

    Full Text Available Avaliou-se o efeito de diferentes níveis de fibra em detergente neutro (FDN, na dieta sobre o comportamento ingestivo de cordeiros Ile de France x Texel. Foram utilizados 20 cordeiros distribuídos em um delineamento experimental inteiramente casualizado, em um total de quatro tratamentos com cinco repetições, e alimentados à vontade com dietas que continham 25%, 31%, 37% e 43% de FDN. Foi utilizada uma ração em mistura completa de silagem de sorgo (AG 2005E e mistura concentrada constituída por farelo de soja, grão de milho quebrado e mistura mineral. As dietas eram isoprotéicas contendo 17% de PB. As dietas foram fornecidas duas vezes ao dia, às 8:00 e às 16:00 horas. O comportamento ingestivo foi determinado mediante observação visual, ocorrido durante 24 horas, a intervalos de 5 minutos, para se determinar o tempo despendido em alimentação, ruminação e ócio. O aumento do teor de fibra na ração não influenciou significativamente (P>0,05 os tempos despendidos em alimentação, ruminação, ócio e tempo de mastigação total. Houve efeito linear crescente sobre as variáveis eficiência de alimentação e de ruminação de FDN (P>0,05. Os ovinos confinados possuem hábito de alimentação predominantemente diurno e de ruminação noturno.The effect of different neutral detergent fiber (NDF levels in the diet on the Ile de France x Texel lambs ingestive behavior was evaluated. Twenty lambs distributed in a fully randomized experimental design were used, in a total of four treatments and five repetitions, fed ad libitum with 25%, 31%, 37% and 43% NDF diets. A ration in a complete mixing in sorghum silage (AG 2005 E and concentrate mixing of soybean meal, fragmented corn grains and mineral mixing was used. The diets were isoproteic (17% crude protein and were given twice a day, at 8 AM and 4 PM. The ingestive behavior was determined by observation, during 24 hours with 5 minutes intervals, to determine the time spent in

  1. Efeito da irradiação e do armazenamento na disponibilidade de ferro em carne de cordeiro tratado com diferentes dietas Effect of irradiation and storage in the iron availability in lamb meat treated with different diets

    Directory of Open Access Journals (Sweden)

    Adriana Régia Marques de Souza

    2008-12-01

    Full Text Available A irradiação é um método eficiente para aumentar a segurança microbiológica e preservar os nutrientes contidos nas carnes, entre eles o ferro. A forma de melhor absorção, ferro heme, deve ser preservada, havendo melhora na qualidade nutricional da carne armazenada. A dieta também pode influenciar nos teores e formas em que são encontrados os nutrientes na carne. O ferro é fornecido pela dieta, sendo essencial para os processos metabólicos como transporte de oxigênio, metabolismo oxidativo e crescimento celular. Amostras de carne de cordeiro tratado com diferentes dietas (controle, TAC1, TAC2 e sorgo, foram embaladas a vácuo, e irradiadas nas doses 0, 2 e 4 kGy, usando-se Irradiador Multipropósito com fonte de cobalto-60 (60Co e armazenadas a 4 °C por 15 dias. Os valores de ferro total e ferro heme foram medidos aos 0 e 15 dias de armazenamento. O armazenamento diminuiu os teores de ferro total (de 18,36 para 14,28 mg.100 g-1 e de ferro heme (de 13,78 para 10,52 mg.100 g-1. As dietas afetaram os níveis de ferro total e heme da carne, sendo que a dieta com sorgo foi a que apresentou maiores teores. A dose de 2 kGy foi a dose que mais afetou os valores de ferro, independentemente dos tempos de armazenamento. Foi constatado que os teores de ferro total e heme variaram em função do tempo de armazenamento, das doses de irradiação e das dietas fornecidas aos cordeiros.Irradiation is an efficient method to increase the microbiological safety and to maintain the nutrients such as iron in the meat. The best absorption form, heme iron, should be preserved in order to increase the nutritional quality of stored meat. The diet can alter the nutrients contents and form in the meat. The iron is provided from the diet and it is an essential element for the metabolic processes such as oxygen transport, oxidative metabolism, and cellular growth. Meat lamb samples treated with different diets (it controls, TAC1, TAC2 and sorghum were wrapped to

  2. The panchromatic spectroscopic evolution of the classical CO nova V339 Delphini (Nova Del 2013) until X-ray turnoff

    Science.gov (United States)

    Shore, S. N.; Mason, E.; Schwarz, G. J.; Teyssier, F. M.; Buil, C.; De Gennaro Aquino, I.; Page, K. L.; Osborne, J. P.; Scaringi, S.; Starrfield, S.; van Winckel, H.; Williams, R. E.; Woodward, C. E.

    2016-05-01

    Context. Classical novae are the product of thermonuclear runaway-initiated explosions occurring on accreting white dwarfs. Aims: V339 Del (Nova Delphinus 2013) was one of the brightest classical novae of the last hundred years. Spectroscopy and photometry are available from γ-rays through infrared at stages that have frequently not been observed well. The complete data set is intended to provide a benchmark for comparison with modeling and for understanding more sparsely monitored historical classical and recurrent novae. This paper is the first in the series of reports on the development of the nova. We report here on the early stages of the outburst, through the X-ray active stage. Methods: A time sequence of optical, flux calibrated high resolution spectra was obtained with the Nordic Optical Telescope (NOT) using FIES simultaneously, or contemporaneously, with the Space Telescope Imaging Spectrograph (STIS) aboard the Hubble Space Telescope during the early stages of the outburst. These were supplemented with Mercator/HERMES optical spectra. High resolution IUE ultraviolet spectra of OS And 1986, taken during the Fe curtain phase, served as a template for the distance determination. We used standard plasma diagnostics (e.g., [O III] and [N II] line ratios, and the Hβ line flux) to constrain electron densities and temperatures of the ejecta. Using Monte Carlo modeling of the ejecta, we derived the structure, filling factor, and mass from comparisons of the optical and ultraviolet line profiles. Results: We derive an extinction of E(B - V) = 0.23 ± 0.05 from the spectral energy distribution, the interstellar absorption, and H I emission lines. The distance, about 4-4.5 kpc, is in agreement with the inferred distance from near infrared interferometry. The maximum velocity was about 2500 km s-1, measured from the UV resonance and optical profiles. The ejecta showed considerable fine structure in all transitions, much of which persisted as emission knots. The

  3. Efeito da restrição alimentar durante o final da gestação sobre o peso ao nascer de cordeiros Santa Inês Effects of maternal undernutrition during final pregnancy on weight birth of Santa Ines lambs

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    Luciana Castro Geraseev

    2006-04-01

    Full Text Available O experimento foi conduzido no setor de Ovinocultura da Universidade Federal de Lavras, com o objetivo de avaliar o peso ao nascer de cordeiros da raça Santa Inês, machos e fêmeas, nascidos de ovelhas submetidas ou não a uma restrição alimentar durante o terço final da gestação. Para tanto, foram utilizadas 44 ovelhas Santa Inês gestando gêmeos, as quais com 100 dias de gestação, foram confinadas e divididas em dois grupos: um grupo recebeu alimentação à vontade para satisfazer suas necessidades energéticas, e o segundo grupo recebeu alimentação restrita para satisfazer 60% das suas necessidades energéticas. O cálculo das necessidades energéticas foi baseado nas recomendações do ARC (1980, levando-se em consideração o peso da ovelha, o tempo de gestação e o número de fetos que cada ovelha estava gestando. Com relação as ovelhas, foram avaliados o peso corporal no início do experimento e logo após a parição, a duração da gestação e a massa biológica produzida. Com relação aos cordeiros, foram avaliados o peso ao nascer dos mesmos, sendo que para tanto estes animais foram divididos de acordo com o sexo (machos e fêmeas. O peso ao nascer dos cordeiros machos e fêmeas foi afetado pela restrição pré-natal, sendo que a média do peso ao nascer dos cordeiros machos sem restrição foi 4,162 kg e com restrição 2,893 kg; e o peso ao nascer das cordeiras fêmeas sem restrição foi 3,474 kg e com restrição 2,855 kg. A grande redução observada neste trabalho no peso ao nascer dos cordeiros machos (30,5% e fêmeas (17,8% revela a importância da adoção de um nível nutricional adequado para as ovelhas gestantes, principalmente durante o terço final da gestação.An experiment was conducted in the Sheep Production Sector of the Animal Science Department at the Federal University of Lavras, Lavras MG to evaluate weight birth of Santa Ines lambs, males and females from ewes submitted or not to feed

  4. Características das fibras musculares de cordeiros nascidos de ovelhas recebendo suplementação proteica no terço inicial da gestação Characteristics of muscle fibers of lambs born from sheep given protein suplementation in the intial third of pregnancy

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    Graziela Aparecida Santello

    2010-10-01

    Full Text Available Foram utilizadas 80 ovelhas Santa Inês, com 47,49 ± 3,76 kg de peso vivo, cobertas com reprodutores Dorper e alimentadas com concentrado com 15,20; 22,48; 26,52 e 35,65% de proteína bruta (PB no terço inicial de gestação. As ovelhas, durante o dia, permaneceram em pastagem de capim-aruana (Panicum maximum cv. Aruana. Ao nascimento, foram realizadas biópsias no músculo Semitendinosus esquerdo de cordeiros machos, para avaliar o número e o diâmetro das fibras musculares. Na fase de terminação, os cordeiros foram distribuídos em dois grupos e alimentados com uma dieta controle, contendo 16,18% de proteína bruta (PB e 79,64% nutrientes digestíveis totais (NDT, sem grão de girassol; ou com uma dieta contendo 9,10% de grãos de girassol (15,03% de PB e 78,96% de NDT. Não houve efeito da alimentação materna sobre o peso dos cordeiros ao nascimento (4,82 kg, aos 30 dias de idade (9,69 kg e ao desmame (15,38 kg. O sexo influenciou o peso dos cordeiros ao nascimento e ao desmame. O desempenho dos cordeiros na fase de terminação não foi influenciado pela dieta fornecida nessa fase, nem pelo sexo nem pelo manejo alimentar da mãe durante a gestação. Não houve diferença no número (2813,45 nem no diâmetro (13,16 μm das fibras musculares ao nascimento. O teor de PB de dietas para ovelhas no terço inicial da gestação pode ser reduzido, pois essa redução não influencia no diâmetro e número de fibras musculares.It was used 80 Santa Inês ewes with average body weight 47.79 ± 3.76 kg, mated with Dorper rams and fed concentrated diet with 15.20; 22.48; 26.52 and 35.65% crude protein (CP on the initial third of pregnancy. Sheep were kept on aruana grass (Panicum maximum cv. Aruana pasture during the day. At birth, biopsy on the left Semitendinosus muscle were done on male lambs to evaluate the number and diameter of muscular fibers. During finishing phase, lambs were distributed in two groups and fed control diet with 16

  5. Intake, apparent digestibility and ruminal characteristics of the lambs fed with increasing levels of concentrate in tropical environment in the Valley of Guaporé - MTConsumo, digestibilidade dos nutrientes e características ruminais de cordeiros alimentados com níveis crescentes de concentrado em ambiente tropical no Vale do Alto Guaporé - MT

    Directory of Open Access Journals (Sweden)

    Luiz Juliano Valério Geron

    2013-10-01

    Full Text Available The objective was to evaluate the use of concentrate in the diet of lambs on intake and total digestibility coefficient (DC of nutrients, ruminal characteristics, rectal and body temperature. It was used four lambs without breed defined (SRD, entire, with average body weight (BW of 19.3 ± 2.07 kg using a Latin square design, 4 x 4. The animals were housed in metabolism cages and were fed twice a day with diet consisting of corn silage and concentrate at a ratio of 20, 40, 60 and 80% dry matter in the diet, composite of corn grains and soybean meal. Leftovers were measured daily and the feces were collected through bags. Data from variables studied were submitted to ANOVA and regression analysis at 5% probability. The increasing levels of concentrate in lamb diets affected (P0.05 of concentrate levels on digestibility coefficient of DM, OM, EE, NDF, ADF, NFC and TCH. However, the digestibility coefficient of CP showed a quadratic effect (P0.05 by dietary concentrate. It can be concluded that 38% of concentrate in diets of lambs favors the maximum dry matter intake, organic matter and crude protein. The digestibility coefficient of the nutrients, except for protein, are not altered with the addition up to 80% concentrate in diet for lambs, as well as, this does not affect the pH and ammonia nitrogen concentration of ruminal fluid, rectal and body temperature. Objetivou-se avaliar níveis crescentes de concentrado na dieta de cordeiros sobre o consumo e coeficiente de digestibilidade total (CD dos nutrientes, características ruminais, temperatura corporal e retal. Foram utilizados quatro cordeiros sem raça definida (SRD, não castrados, com peso corporal (PC médio de 19,3 Kg ± 2,07 por meio de um delineamento em quadrado latino 4 x 4. Os animais foram alojados em gaiolas de metabolismo, os quais foram alimentados duas vezes ao dia, com dieta composta por silagem de milho e concentrado, na proporção de 20, 40, 60 e 80% na matéria seca da

  6. Temperamento e comportamento materno-filial de ovinos das raças Corriedale e Ideal e sua relação com a sobrevivência dos cordeiros Temperament and maternal behavior of Corriedale and Pollwarth sheep and its relation with lamb's survival

    Directory of Open Access Journals (Sweden)

    Carmen Lucia de Souza Rech

    2008-08-01

    Full Text Available O experimento foi conduzido na Estação Experimental da Embrapa, Bagé, Rio Grande do Sul, entre março de 2005 e fevereiro de 2006. O objetivo foi avaliar o comportamento materno-filial e o temperamento de ovelhas e cordeiros e relacioná-los com a sobrevivência dos cordeiros. Foram utilizadas 47 ovelhas da raça Corriedale, com peso médio de 52,1kg, e 45 ovelhas da raça Ideal, com peso médio de 49,5kg, em um delineamento inteiramente casualizado. O temperamento foi avaliado por meio dos testes: escore de comportamento materno (ECM, tempo de fuga, tipo de marcha e distância de fuga. As ovelhas da raça Corriedale apresentaram maiores valores no teste tipo de marcha que as ovelhas da raça Ideal. Os cordeiros da raça Corriedale eram os mais pesados e tinham maior índice de sobrevivência, quando comparados com os da raça Ideal. A raça não afetou o escore de comportamento materno. Ovelhas reativas (ECM=1, que fogem e não retornam aos seus cordeiros, se isolaram menos do rebanho antes do parto, protegeram menos suas crias, desmamaram-nas mais cedo e tiveram menor peso em relação às não-reativas. A reatividade das ovelhas prejudicou o cuidado materno com os cordeiros e essa característica deve ser considerada pelo setor produtivo.The trial was conducted at the Experimental Station of Embrapa, Bagé, RS, from March 2005 to February 2006, and aimed to evaluate the maternal behavior and temperament of ewes and their lambs and related them with lamb's survival. Forty-seven Corriedale ewes with mean body weight of 52.1kg and 45 Pollwarth ewes with mean body weight of 49.5kg were used, according to a completely randomized design. Temperament was evaluated through maternal behaviour score (MBS, flight time test (score and quantitative and flight distance. Corriedale ewes presented larger values for flight time score than Pollwarth ewes. Corriedale lambs were heavier and a greater number survived than Pollwarth lambs. Sheep breed did not

  7. Substituição do milho por polpa cítrica em rações com alta proporção de concentrado para cordeiros confinados Replacement of corn by citrus pulp in high grain diets fed to feedlot lambs

    Directory of Open Access Journals (Sweden)

    Gustavo Henrique Rodrigues

    2008-06-01

    Full Text Available A polpa cítrica desidratada (PC é um subproduto altamente energético e com potencial para substituir o milho em rações de cordeiros desmamados precocemente. Dois experimentos foram realizados para avaliarem-se os efeitos da substituição do milho por PC no desempenho de cordeiros e na digestibilidade das rações. No Experimento 1, 64 cordeiros Santa Inês, com peso vivo inicial de 18 (±0,6 kg e 73 (±1 dias de idade, foram utilizados para avaliar o ganho de peso médio diário (GMD, o consumo de matéria seca (CMS e a conversão alimentar (CA. No experimento 2, 12 cordeiros foram mantidos em gaiolas para ensaio de metabolismo para determinar a digestibilidade aparente das rações no trato digestório total e o metabolismo de nitrogênio. Nos dois experimentos, os cordeiros foram alimentados com uma ração contendo 90% de concentrado (milho moído e/ou PC, farelo de soja e minerais e 10% de feno de "coastcross" (Cynodon spp. A PC foi adicionada em 23,7; 46,1 e 68,4% da MS, substituindo o milho em 33, 67 e 100%, respectivamente. No Experimento 1, foi observado a maximização do GMD (267g dia-1 e do CMS (1,01kg dia-1, até o teor de substituição de 33% do milho pela PC. No Experimento 2, houve efeito linear (P0,05 entre os tratamentos na digestiblidade aparente da matéria orgânica e no balanço de nitrogênio.Dried citrus pulp (DCP is a high energy byproduct and may be used to replace corn in early weaned lamb diets. Two trials were performed to evaluate the effects of replacing corn by dried citrus pulp on lamb performance and diet digestibility. In trial 1, 64 Santa Ines ram lambs (initial BW 18 ± 0.6kg and 73 ± 1 days old were used to evaluate average daily gain (ADG, dry matter intake (DMI and feed conversion (FC. In trial 2, 12 ram lambs were placed in metabolism crates to evaluate N metabolism and apparent digestibility of diets. In both trials, lambs were fed a 90% concentrate (ground corn and/or DCP, soybean meal and

  8. Composição tecidual e perfil de ácidos graxos do lombo de cordeiros terminados em pasto com níveis de suplementação concentrada Tissue composition and fatty acids profile of lambs loin finishing on pasture with concentrate supplementation

    Directory of Open Access Journals (Sweden)

    Maria Angela Machado Fernandes

    2009-11-01

    Full Text Available A composição tecidual da carne é característica importante na avaliação da qualidade sensorial e nutricional do produto. O presente trabalho avaliou a composição tecidual e o perfil de ácidos graxos do lombo de cordeiros desmamados aos 42 dias de idade média e terminados em pasto de azevém com níveis diários de suplementação concentrada (0, 1 e 2% do PV e ad libitum. O delineamento experimental foi de blocos ao acaso com três repetições. Os cordeiros foram abatidos ao atingirem 32kg de peso vivo. O lombo direito foi utilizado para determinação da composição tecidual e o esquerdo para análise de perfil de ácidos graxos. As análises de variância e de regressão foram realizadas com auxílio do programa SAS (2001. A suplementação concentrada de cordeiros terminados em pasto não teve efeito (P>0,05 sobre o desenvolvimento muscular e ósseo; no entanto, promoveu acréscimo linear na deposição de gordura intermuscular e total. Os níveis de suplementação estudados não tiveram efeito (P>0,05 sobre a quantidade e o percentual de cada ácido graxo da carne dos cordeiros. A suplementação concentrada de cordeiros desmamados em pasto de azevém aumentou a deposição de gordura na carcaça sem afetar a qualidade da carne para o consumo humano, considerando-se o perfil de ácidos graxos.Meat composition is an important aspect on evaluation of sensory and nutritional quality of the product. This work had the objective of evaluating tissue composition and fatty acids profile of loin lambs weaned at 42 days of mean age and finished on ryegrass pasture with levels (0%; 1% and 2% of BW; ad libitum of daily concentrate supplementation. The experiment was allocated in randomized blocks design with three replications. Lambs were slaughtered when individual live weight reached 32kg. Tissue composition was determined in right loin and left loin was used for fatty acids profile analyses. Analysis of variance and regression were

  9. Características físico-químicas e sensoriais da carne de cordeiros terminados com dietas contendo cana-de-açúcar ou silagem de milho e dois níveis de concentrado Physic-chemical and sensorial characteristics of meat from lambs finished with diets containing sugar cane or corn silage and two levels of concentrate

    Directory of Open Access Journals (Sweden)

    André Gustavo Leão

    2012-05-01

    Full Text Available Com o objetivo de avaliar as características físico-químicas e sensoriais da carne de cordeiros terminados em confinamento com dietas contendo cana-de-açúcar ou silagem de milho em duas relações volumoso:concentrado, 60:40 ou 40:60, utilizaram-se 32 cordeiros Ile de France, não-castrados, com 15 kg de peso corporal. Os animais foram confinados em baias individuais e abatidos aos 32 kg. As dietas e os músculos estudados não influenciaram o pH aos 45 minutos (6,56 e 24 horas (5,62 após o abate nem a capacidade de retenção de água (58,38% e a perda de peso por cocção (34,04%. A cor da carne e da gordura subcutânea não diferiu entre as dietas, entretanto a cor da carne variou entre os músculos longissimus lumborum e triceps brachii. A força de cisalhamento (1,85 kgf/cm² não foi afetada pelas dietas, porém diferiu entre os músculos, com valores de 1,41 e 2,28 kgf/cm² para o longissimus lumborum e triceps brachii, respectivamente. Nas análises sensoriais do lombo e da paleta, foram obtidas para os cordeiros alimentados com cana-de-açúcar e maior quantidade de concentrado as maiores notas para sabor (8,07 e 8,26, textura (8,53 e 8,53, preferência (8,20 e 8,46 e aceitação (8,33 e 8,26, respectivamente. A cana-de-açúcar na alimentação de cordeiros em confinamento manteve a qualidade físicoquímica da carne, podendo ser utilizada nesta fase de produção e, quando associada a maior quantidade de concentrado na dieta, melhora a qualidade sensorial da carne de cordeiros.With the objective of evaluating physic-chemical and sensorial characteristics of meat from lambs finished in feedlot with diets containing sugar cane or corn silage at two roughage:concentrate ratios, 60:40 or 40:60, 32 non-castrated Ile de France lambs, with 15 kg body weight were used. Animals were confined in individual stalls and were slaughtered at 32 kg body weight. Studied diets and muscles did not affect pH at 45 minutes (6.56 and 24 hours (5

  10. The Radio Light Curve of the Gamma-Ray Nova in V407 CYG: Thermal Emission from the Ionized Symbiotic Envelope, Devoured from Within by the Nova Blast

    Science.gov (United States)

    Chomiuk, Laura; Krauss, Miriam I.; Rupen, Michael P.; Nelson, Thomas; Roy, Nirupam; Sokoloski, Jennifer L.; Mukai, Koji; Munari, Ulisse; Mioduszewski, Amy; Weston, Jeninfer; O'Brien, Tim J.; Eyres, Steward P. S.; Bode, Michael F.

    2012-01-01

    We present multi-frequency radio observations of the 2010 nova event in the symbiotic binary V407 Cygni, obtained with the Karl G. Jansky Very Large Array (VLA) and spanning 1.45 GHz and 17.770 days following discovery. This nova.the first ever detected in gamma rays.shows a radio light curve dominated by the wind of the Mira giant companion, rather than the nova ejecta themselves. The radio luminosity grewas the wind became increasingly ionized by the nova outburst, and faded as the wind was violently heated from within by the nova shock. This study marks the first time that this physical mechanism has been shown to dominate the radio light curve of an astrophysical transient. We do not observe a thermal signature from the nova ejecta or synchrotron emission from the shock, due to the fact that these components were hidden behind the absorbing screen of the Mira wind. We estimate a mass-loss rate for the Mira wind of .Mw approximately equals 10(exp -6) Solar mass yr(exp -1). We also present the only radio detection of V407 Cyg before the 2010 nova, gleaned from unpublished 1993 archival VLA data, which shows that the radio luminosity of the Mira wind varies by a factor of 20 even in quiescence. Although V407 Cyg likely hosts a massive accreting white dwarf, making it a candidate progenitor system for a Type Ia supernova, the dense and radially continuous circumbinary material surrounding V407 Cyg is inconsistent with observational constraints on the environments of most Type Ia supernovae.

  11. The local stellar population of novae regions in the Large Magellanic Cloud

    CERN Document Server

    Subramanian, A; Subramaniam, Annapurni

    2002-01-01

    The distribution of novae across the face of the Large Magellanic Cloud (LMC) and star formation history (SFH) of nearby regions around them are presented using photometric data of stars and star clusters in the OGLE II survey and star cluster catalogues. The nova population in the LMC belong, predominantly to the fast category, with only 11.8% belonging to the slow nova population. All the novae detected within the Bar are fast novae.The age of the stellar population within a few arcmin around novae regions are estimated using isochrone fits to the V vs (V-I) colour-magnitude diagrams. Of the 15 regions studied, excepting the one around the slow nova, all the other regions do not show stellar population in the range 4 - 10 Gyr and the star formation is found to have started between 4 - 2.0 Gyr, with a majority of regions starting the star formation at 3.2 Gyr. This star formation event lasted until 1.6 - 1.8 Gyr. Based on the SFH, it is estimated that the parent population of the fast and moderately fast nov...

  12. Constraining nova observables: direct measurements of resonance strengths in 33S(p,\\gamma)34Cl

    CERN Document Server

    Fallis, J; Bertone, P F; Bishop, S; Buchmann, L; Chen, A A; Christian, G; Clark, J A; D'Auria, J M; Davids, B; Deibel, C M; Fulton, B R; Greife, U; Guo, B; Hager, U; Herlitzius, C; Hutcheon, D A; José, J; Laird, A M; Li, E T; Li, Z H; Lian, G; Liu, W P; Martin, L; Nelson, K; Ottewell, D; Parker, P D; Reeve, S; Rojas, A; Ruiz, C; Setoodehnia, K; Sjue, S; Vockenhuber, C; Wang, Y B; Wrede, C

    2013-01-01

    The 33S(p,\\gamma)34Cl reaction is important for constraining predictions of certain isotopic abundances in oxygen-neon novae. Models currently predict as much as 150 times the solar abundance of 33S in oxygen-neon nova ejecta. This overproduction factor may, however, vary by orders of magnitude due to uncertainties in the 33S(p,\\gamma)34Cl reaction rate at nova peak temperatures. Depending on this rate, 33S could potentially be used as a diagnostic tool for classifying certain types of presolar grains. Better knowledge of the 33S(p,\\gamma)34Cl rate would also aid in interpreting nova observations over the S-Ca mass region and contribute to the firm establishment of the maximum endpoint of nova nucleosynthesis. Additionally, the total S elemental abundance which is affected by this reaction has been proposed as a thermometer to study the peak temperatures of novae. Previously, the 33S(p,\\gamma)34Cl reaction rate had only been studied directly down to resonance energies of 432 keV. However, for nova peak temper...

  13. The 30P(p, γ31S reaction in classical novae: progress and prospects

    Directory of Open Access Journals (Sweden)

    C. Wrede

    2014-01-01

    Full Text Available The unknown thermonuclear rate of the 30P(p, γ31S reaction at classical-nova temperatures currently prohibits the accurate modeling of nova nucleosynthesis in the A ⩾ 30 region. This is hindering the calibration of nova thermometers based on observed O/S, S/Al, O/P, and P/Al abundance ratios in nova ejecta, the calibration of a meter to probe mixing at the core-envelope interface in novae based on the observed Si/H abundance ratio, and the identification of candidate pre-solar nova grains found in primitive meteorites based on laboratory measurements of their 30Si/28Si isotopic ratios. Each of these diagnostics could address key questions in our understanding of classical novae if the 30P(p, γ31S rate were known. We review progress on the determination of the 30P(p, γ31S rate leading to a critical assessment of current interpretations of published data and prospects for future work.

  14. First Measurement of Electron Neutrino Appearance in NOvA.

    Science.gov (United States)

    Adamson, P; Ader, C; Andrews, M; Anfimov, N; Anghel, I; Arms, K; Arrieta-Diaz, E; Aurisano, A; Ayres, D S; Backhouse, C; Baird, M; Bambah, B A; Bays, K; Bernstein, R; Betancourt, M; Bhatnagar, V; Bhuyan, B; Bian, J; Biery, K; Blackburn, T; Bocean, V; Bogert, D; Bolshakova, A; Bowden, M; Bower, C; Broemmelsiek, D; Bromberg, C; Brunetti, G; Bu, X; Butkevich, A; Capista, D; Catano-Mur, E; Chase, T R; Childress, S; Choudhary, B C; Chowdhury, B; Coan, T E; Coelho, J A B; Colo, M; Cooper, J; Corwin, L; Cronin-Hennessy, D; Cunningham, A; Davies, G S; Davies, J P; Del Tutto, M; Derwent, P F; Deepthi, K N; Demuth, D; Desai, S; Deuerling, G; Devan, A; Dey, J; Dharmapalan, R; Ding, P; Dixon, S; Djurcic, Z; Dukes, E C; Duyang, H; Ehrlich, R; Feldman, G J; Felt, N; Fenyves, E J; Flumerfelt, E; Foulkes, S; Frank, M J; Freeman, W; Gabrielyan, M; Gallagher, H R; Gebhard, M; Ghosh, T; Gilbert, W; Giri, A; Goadhouse, S; Gomes, R A; Goodenough, L; Goodman, M C; Grichine, V; Grossman, N; Group, R; Grudzinski, J; Guarino, V; Guo, B; Habig, A; Handler, T; Hartnell, J; Hatcher, R; Hatzikoutelis, A; Heller, K; Howcroft, C; Huang, J; Huang, X; Hylen, J; Ishitsuka, M; Jediny, F; Jensen, C; Jensen, D; Johnson, C; Jostlein, H; Kafka, G K; Kamyshkov, Y; Kasahara, S M S; Kasetti, S; Kephart, K; Koizumi, G; Kotelnikov, S; Kourbanis, I; Krahn, Z; Kravtsov, V; Kreymer, A; Kulenberg, Ch; Kumar, A; Kutnink, T; Kwarciancy, R; Kwong, J; Lang, K; Lee, A; Lee, W M; Lee, K; Lein, S; Liu, J; Lokajicek, M; Lozier, J; Lu, Q; Lucas, P; Luchuk, S; Lukens, P; Lukhanin, G; Magill, S; Maan, K; Mann, W A; Marshak, M L; Martens, M; Martincik, J; Mason, P; Matera, K; Mathis, M; Matveev, V; Mayer, N; McCluskey, E; Mehdiyev, R; Merritt, H; Messier, M D; Meyer, H; Miao, T; Michael, D; Mikheyev, S P; Miller, W H; Mishra, S R; Mohanta, R; Moren, A; Mualem, L; Muether, M; Mufson, S; Musser, J; Newman, H B; Nelson, J K; Niner, E; Norman, A; Nowak, J; Oksuzian, Y; Olshevskiy, A; Oliver, J; Olson, T; Paley, J; Pandey, P; Para, A; Patterson, R B; Pawloski, G; Pearson, N; Perevalov, D; Pershey, D; Peterson, E; Petti, R; Phan-Budd, S; Piccoli, L; Pla-Dalmau, A; Plunkett, R K; Poling, R; Potukuchi, B; Psihas, F; Pushka, D; Qiu, X; Raddatz, N; Radovic, A; Rameika, R A; Ray, R; Rebel, B; Rechenmacher, R; Reed, B; Reilly, R; Rocco, D; Rodkin, D; Ruddick, K; Rusack, R; Ryabov, V; Sachdev, K; Sahijpal, S; Sahoo, H; Samoylov, O; Sanchez, M C; Saoulidou, N; Schlabach, P; Schneps, J; Schroeter, R; Sepulveda-Quiroz, J; Shanahan, P; Sherwood, B; Sheshukov, A; Singh, J; Singh, V; Smith, A; Smith, D; Smolik, J; Solomey, N; Sotnikov, A; Sousa, A; Soustruznik, K; Stenkin, Y; Strait, M; Suter, L; Talaga, R L; Tamsett, M C; Tariq, S; Tas, P; Tesarek, R J; Thayyullathil, R B; Thomsen, K; Tian, X; Tognini, S C; Toner, R; Trevor, J; Tzanakos, G; Urheim, J; Vahle, P; Valerio, L; Vinton, L; Vrba, T; Waldron, A V; Wang, B; Wang, Z; Weber, A; Wehmann, A; Whittington, D; Wilcer, N; Wildberger, R; Wildman, D; Williams, K; Wojcicki, S G; Wood, K; Xiao, M; Xin, T; Yadav, N; Yang, S; Zadorozhnyy, S; Zalesak, J; Zamorano, B; Zhao, A; Zirnstein, J; Zwaska, R

    2016-04-15

    We report results from the first search for ν_{μ}→ν_{e} transitions by the NOvA experiment. In an exposure equivalent to 2.74×10^{20} protons on target in the upgraded NuMI beam at Fermilab, we observe 6 events in the Far Detector, compared to a background expectation of 0.99±0.11(syst) events based on the Near Detector measurement. A secondary analysis observes 11 events with a background of 1.07±0.14(syst). The 3.3σ excess of events observed in the primary analysis disfavors 0.1π<δ_{CP}<0.5π in the inverted mass hierarchy at the 90% C.L.

  15. First Measurement of Electron Neutrino Appearance in NOvA

    Science.gov (United States)

    Adamson, P.; Ader, C.; Andrews, M.; Anfimov, N.; Anghel, I.; Arms, K.; Arrieta-Diaz, E.; Aurisano, A.; Ayres, D. S.; Backhouse, C.; Baird, M.; Bambah, B. A.; Bays, K.; Bernstein, R.; Betancourt, M.; Bhatnagar, V.; Bhuyan, B.; Bian, J.; Biery, K.; Blackburn, T.; Bocean, V.; Bogert, D.; Bolshakova, A.; Bowden, M.; Bower, C.; Broemmelsiek, D.; Bromberg, C.; Brunetti, G.; Bu, X.; Butkevich, A.; Capista, D.; Catano-Mur, E.; Chase, T. R.; Childress, S.; Choudhary, B. C.; Chowdhury, B.; Coan, T. E.; Coelho, J. A. B.; Colo, M.; Cooper, J.; Corwin, L.; Cronin-Hennessy, D.; Cunningham, A.; Davies, G. S.; Davies, J. P.; Del Tutto, M.; Derwent, P. F.; Deepthi, K. N.; Demuth, D.; Desai, S.; Deuerling, G.; Devan, A.; Dey, J.; Dharmapalan, R.; Ding, P.; Dixon, S.; Djurcic, Z.; Dukes, E. C.; Duyang, H.; Ehrlich, R.; Feldman, G. J.; Felt, N.; Fenyves, E. J.; Flumerfelt, E.; Foulkes, S.; Frank, M. J.; Freeman, W.; Gabrielyan, M.; Gallagher, H. R.; Gebhard, M.; Ghosh, T.; Gilbert, W.; Giri, A.; Goadhouse, S.; Gomes, R. A.; Goodenough, L.; Goodman, M. C.; Grichine, V.; Grossman, N.; Group, R.; Grudzinski, J.; Guarino, V.; Guo, B.; Habig, A.; Handler, T.; Hartnell, J.; Hatcher, R.; Hatzikoutelis, A.; Heller, K.; Howcroft, C.; Huang, J.; Huang, X.; Hylen, J.; Ishitsuka, M.; Jediny, F.; Jensen, C.; Jensen, D.; Johnson, C.; Jostlein, H.; Kafka, G. K.; Kamyshkov, Y.; Kasahara, S. M. S.; Kasetti, S.; Kephart, K.; Koizumi, G.; Kotelnikov, S.; Kourbanis, I.; Krahn, Z.; Kravtsov, V.; Kreymer, A.; Kulenberg, Ch.; Kumar, A.; Kutnink, T.; Kwarciancy, R.; Kwong, J.; Lang, K.; Lee, A.; Lee, W. M.; Lee, K.; Lein, S.; Liu, J.; Lokajicek, M.; Lozier, J.; Lu, Q.; Lucas, P.; Luchuk, S.; Lukens, P.; Lukhanin, G.; Magill, S.; Maan, K.; Mann, W. A.; Marshak, M. L.; Martens, M.; Martincik, J.; Mason, P.; Matera, K.; Mathis, M.; Matveev, V.; Mayer, N.; McCluskey, E.; Mehdiyev, R.; Merritt, H.; Messier, M. D.; Meyer, H.; Miao, T.; Michael, D.; Mikheyev, S. P.; Miller, W. H.; Mishra, S. R.; Mohanta, R.; Moren, A.; Mualem, L.; Muether, M.; Mufson, S.; Musser, J.; Newman, H. B.; Nelson, J. K.; Niner, E.; Norman, A.; Nowak, J.; Oksuzian, Y.; Olshevskiy, A.; Oliver, J.; Olson, T.; Paley, J.; Pandey, P.; Para, A.; Patterson, R. B.; Pawloski, G.; Pearson, N.; Perevalov, D.; Pershey, D.; Peterson, E.; Petti, R.; Phan-Budd, S.; Piccoli, L.; Pla-Dalmau, A.; Plunkett, R. K.; Poling, R.; Potukuchi, B.; Psihas, F.; Pushka, D.; Qiu, X.; Raddatz, N.; Radovic, A.; Rameika, R. A.; Ray, R.; Rebel, B.; Rechenmacher, R.; Reed, B.; Reilly, R.; Rocco, D.; Rodkin, D.; Ruddick, K.; Rusack, R.; Ryabov, V.; Sachdev, K.; Sahijpal, S.; Sahoo, H.; Samoylov, O.; Sanchez, M. C.; Saoulidou, N.; Schlabach, P.; Schneps, J.; Schroeter, R.; Sepulveda-Quiroz, J.; Shanahan, P.; Sherwood, B.; Sheshukov, A.; Singh, J.; Singh, V.; Smith, A.; Smith, D.; Smolik, J.; Solomey, N.; Sotnikov, A.; Sousa, A.; Soustruznik, K.; Stenkin, Y.; Strait, M.; Suter, L.; Talaga, R. L.; Tamsett, M. C.; Tariq, S.; Tas, P.; Tesarek, R. J.; Thayyullathil, R. B.; Thomsen, K.; Tian, X.; Tognini, S. C.; Toner, R.; Trevor, J.; Tzanakos, G.; Urheim, J.; Vahle, P.; Valerio, L.; Vinton, L.; Vrba, T.; Waldron, A. V.; Wang, B.; Wang, Z.; Weber, A.; Wehmann, A.; Whittington, D.; Wilcer, N.; Wildberger, R.; Wildman, D.; Williams, K.; Wojcicki, S. G.; Wood, K.; Xiao, M.; Xin, T.; Yadav, N.; Yang, S.; Zadorozhnyy, S.; Zalesak, J.; Zamorano, B.; Zhao, A.; Zirnstein, J.; Zwaska, R.; NOvA Collaboration

    2016-04-01

    We report results from the first search for νμ→νe transitions by the NOvA experiment. In an exposure equivalent to 2.74 ×1020 protons on target in the upgraded NuMI beam at Fermilab, we observe 6 events in the Far Detector, compared to a background expectation of 0.99 ±0.11 (syst) events based on the Near Detector measurement. A secondary analysis observes 11 events with a background of 1.07 ±0.14 (syst) . The 3.3 σ excess of events observed in the primary analysis disfavors 0.1 π <δC P<0.5 π in the inverted mass hierarchy at the 90% C.L.

  16. NSV 1907 - A new eclipsing, nova-like cataclysmic variable

    CERN Document Server

    Hümmerich, Stefan; Hambsch, Franz-Josef; Dubois, Franky; Ashley, Richard; Gänsicke, Boris T; Vanaverbeke, Siegfried; Bernhard, Klaus; Wils, Patrick

    2016-01-01

    NSV 1907, formerly listed as an irregular variable in variability catalogues, was classified as an Algol-type eclipsing binary in the Catalina Surveys Periodic Variable Star Catalogue. We have identified NSV 1907 as an ultraviolet (UV) bright source using measurements from the GALEX space telescope and detected obvious out-of-eclipse variability in archival photometric data from the Catalina Sky Survey, which instigated a closer examination of the object. A spectrum and extensive multicolour photometric observations were acquired, from which we deduce that NSV 1907 is a deeply eclipsing, nova-like cataclysmic variable. Apart from the orbital variations (deep eclipses with a period of P ~ 6.63 hours), changes in mean brightness and irregular short-term variability (flickering) were observed. The presence of a secondary minimum at phase phi ~ 0.5 was established, which indicates a significant contribution of the companion star to the optical flux of the system. We find possible evidence for sinusoidal variation...

  17. Do policial ao noir: as novas faces da narrativa violenta

    Directory of Open Access Journals (Sweden)

    Paulo Sesar Pimentel

    2014-01-01

    Full Text Available O presente artigo se propõe a, num primeiro momento, descrever a evolução do gênero policial, do seu surgimento até sua transformação, numa nova categoria, designada por noir. Partindo deste ponto, trabalham-se as especificidades do chamado romance negro, suas motivações e suas peculiaridades, inseridas na estrutura social contemporânea, discutindo, por sua relação intrínseca, a violência e a morte. A fim de exemplificar esta construção narrativa, usa-se o conto "Tempestade sobre a Montanha", de Wander Antunes, numa análise que permite vislumbrar as manifestações temáticas e estruturais deste novo gênero adaptadas à realidade brasileira.

  18. Corpos e Corporeidade no Universo da Nova Era no Brasil

    Directory of Open Access Journals (Sweden)

    Amurabi Oliveira

    2012-08-01

    Full Text Available O presente trabalho busca explorar a dimensão corpórea enquanto central para a compreensão do fenômeno religioso, em especial do universo Nova Era – NE, em nossa interpretação o corpo apresenta-se enquanto estrutura estruturada estruturante que possibilita aos sujeitos vivenciar e interpretar o mundo, neste sentido, a experiência de imersão e de vivência das práticas da NE são, essencialmente, experiências corpóreas. No decorrer deste trabalho buscaremos dar destaque aos aspectos singulares da NE brasileira, em especial no que tange à dimensão do êxtase sagrado, principalmente a partir do diálogo com as religiões afro-brasileiras.

  19. NOVA: Program Summaries of New Science TV Series.

    Science.gov (United States)

    1974-03-22

    A new science television series now broadcast over the Public Broadcasting Service (PBS) will be of special interest to members of AAAS. The series, called NOVA, is produced by WGBH-TV, Boston, for PBS. The series has been created and produced with the advice and cooperation of AAAS, especially its Committee on the Public Understanding of Science and the Office of Communications Programs, as a major new effort at expanding the public's understanding of science and scientific processes. The series is financed by grants from the Carnegie Corporation of New York, the Corporation for Public Broadcasting, the National Science Foundation, and Polaroid. A list of program descriptions in the current series with network air dates follows. Consult your local listings for local times.

  20. On The Nature Of Superoutbursts In Dwarf Novae

    CERN Document Server

    Truss, M R; Wynn, G A; Truss, Michael; Murray, James; Wynn, Graham

    2001-01-01

    We present the first detailed hydrodynamic simulation of a superoutburst to incorporate the full tidal potential of a binary system. A two-dimensional smoothed particle hydrodynamics code is used to simulate a superoutburst in a binary with the parameters of the SU UMa system Z Chamaeleontis. The simulated light curves shows all the features observed in such systems. Analysis of the mass flux through the disc and the growth rate of the superhumps and disc eccentricity show that the superoutburst-superhump phenomenon is a direct result of tidal instability. No enhanced mass transfer from the secondary is required to initiate or sustain these phenomena. Comparisons of superoutbursts with normal outbursts are made and we show that the model can be reconciled with the behavior of U Geminorum type dwarf novae, which show no superoutbursts.

  1. O superego: em busca de uma nova abordagem

    Directory of Open Access Journals (Sweden)

    Marta Rezende Cardoso

    Full Text Available Este artigo apresenta a proposição de uma nova concepção do superego, segundo a qual os imperativos superegóicos seriam comparáveis, em todos os indivíduos, a um “enclave psicótico”. Trata-se aqui de aprofundar aspectos fundamentais da questão do superego, numa tentativa de elaborar alguns pontos que ficaram problemáticos em Freud, Melanie Klein e outros autores pós-freudianos. A obra de Jean Laplanche foi útil como fonte principal na formulação das hipóteses apresentadas cuja incidência na clínica psicanalítica parece inegável.

  2. High resolution spectra of novae and the quadratic zeeman effect

    Directory of Open Access Journals (Sweden)

    Robert Williams

    2006-01-01

    Full Text Available Los espectros de alta resoluci on de novas despu es de las erupciones revelan caracter sticas distintivas en los per les e intensidades de las l neas. Las l neas de Balmer m as altas son frecuentemente m as anchas que los miembros m as bajos de la serie, y los per les e intensidades relativos del doblete [O I] 6300, 6364 di eren de los valores normales. Nosotros sugerimos que estos aspectos pueden ser producidos por el efecto cuadr atico Zeeman desde campos magn eticos que exceden B=106 gauss. Tomadas juntas, las l neas de emisi on y absorci on indican m ultiples or genes para los materiales expulsados, tanto en las enanas blancas eruptivas como en las estrellas secundarias fr as.

  3. Ten-year literature review of global endometrial ablation with the NovaSure® device

    Directory of Open Access Journals (Sweden)

    Gimpelson RJ

    2014-03-01

    Full Text Available Richard J Gimpelson Mercy Clinic, Minimally Invasive Gynecology, Department of Obstetrics and Gynecology, Mercy Hospital St Louis, St Louis, MO, USA Abstract: This review examines the peer-reviewed literature describing prospective studies that report amenorrhea rates, patient satisfaction, and surgical reintervention rates following the NovaSure® endometrial ablation procedure. A search of the English-language literature published from 2000 to 2011 was conducted using PubMed. Ten prospective studies, six single-arm NovaSure trials, and four randomized controlled trials comparing the NovaSure procedure with other global endometrial ablation modalities met the inclusion criteria and were reviewed. The follow-up periods ranged from 6 to 60 months. Amenorrhea rates for the NovaSure procedure ranged from 30.0% to 75.0%. Patients who reported being satisfied with the NovaSure procedure ranged from 85.0% to 94.0%. In randomized controlled trials with other global endometrial ablation modalities, amenorrhea rates at 12 months with the NovaSure procedure ranged from 43.0% to 56.0%, while other modalities ranged from 8% to 24%. In addition, this manuscript reviews the following: the NovaSure technology; use of the NovaSure procedure in the office setting; intraoperative and postoperative pain; effects on premenstrual syndrome (PMS; dysmenorrhea; special circumstances, including presence of uterine disease, history of cesarean delivery, coagulopathy, or use of anticoagulant medication; post-procedure uterine cavity assessment and cancer risk; contraception and pregnancy; and safety. Keywords: abnormal uterine bleeding, menorrhagia, endometrial ablation, NovaSure®

  4. Sobre el Grup de Sabadell y los Nova Novorum

    Directory of Open Access Journals (Sweden)

    Pego Puigbó, Armando

    2011-12-01

    Full Text Available In the present paper, from a comparative point of view, the literary roots of two of the most outstanding proposals for the renewal of the Spanish and Catalan narratives in the twenties and thirties are tried to describe. It is possible to find out the parallelisms between the work of Antonio Espina and Francesc Trabal in the dialogue with the aesthetical experience of the European vanguards to which they are linked by the narrative folly of their own contracdictions. Having in consideration the possibilities offered by the poem in prose or the microromance, similar responses could be traced between the «Grup of Sabadell» and the «Nova Novarum». In this way, Pájaro Pinto (1927 and Luna de copas (1929, by Espina, and L’ home que es va perdre (1929 or Judita (1939 by Trabal will be analyzed together.En el presente artículo se pretende describir, de manera comparada, las raíces literarias de dos de las propuestas más renovadoras de las narrativas española y catalana de los años veinte y treinta del siglo XX. Cabe buscar los posibles paralelismos entre la obra de Antonio Espina y Francesc Trabal en el diálogo con la experiencia estética de las vanguardias europeas en las que se insertaban y en la exasperación narrativa de sus propias contradicciones. Teniendo en cuenta las posiblilidades que ofrecía el poema en prosa o el microrrelato, será posible rastrear una similitud de respuestas que entrelaza la reflexión del «Grup de Sabadell» con la de los «Nova Novorum». A tal fin, se analizarán conjuntamente Pájaro Pinto (1927 y Luna de copas (1929, de Espina, y L’ home que es va perdre (1929 y Judita (1939 de Trabal.

  5. Novas tecnologias aplicadas às embalagens de alimentos

    Directory of Open Access Journals (Sweden)

    Flávia De Floriani Pozza Rebello

    2009-12-01

    Full Text Available Com o desenvolvimento da indústria de alimentos, as embalagens têm se aperfeiçoado, indo além de sua função básica de proteger o alimento contra danos mecânicos e contaminações químicas e microbiológicas. Elas têm cada vez mais desempenhando papel de destaque, contribuindo ativamente para a venda de um produto. Assim, as indústrias de embalagens têm procurado atender aos consumidores mais exigentes e juntamente aos centros de pesquisa e universidades, têm investido mais em estudos de novas tecnologias, a fim de prolongar as características de qualidade do alimento, conferir melhor aparência, maior proteção mecânica no embarque, transporte, desembarque e nos supermercados, oferecer embalagens mais compactas, que ocupem menos espaço na geladeira, com abertura e fechamento mais fáceis, e que utilizem materiais de fácil reciclagem ou decomposição no ambiente. Com o objetivo de atender às novas expectativas das indústrias de alimentos e dos consumidores, surgem as embalagens ativas e as embalagens inteligentes. As embalagens ativas são aquelas que interagem de alguma forma com o alimento, seja liberando substâncias conservantes ao longo da vida de prateleira do produto, ou “corrigindo” alguns problemas naturais do alimento, como sabor amargo por exemplo, em que algumas enzimas podem ser adicionadas ao material de embalagem, minimizando este problema e tornando o produto mais saboroso. Já as embalagens inteligentes indicam as modificações químicas às quais os alimentos estão passando, como mudanças de pH, por exemplo, indicando alterações na qualidade do produto.

  6. Data Mining for Dwarf Novae in SDSS, GALEX and Astrometric Catalogues

    CERN Document Server

    Wils, Patrick; Drake, Andrew J; Southworth, John

    2009-01-01

    By cross matching blue objects from SDSS with GALEX and the astrometric catalogues USNO-B1.0, GSC2.3 and CMC14, 64 new dwarf nova candidates with one or more observed outbursts have been identified. 14 of these systems are confirmed as cataclysmic variables through existing and follow-up spectroscopy. A study of the amplitude distribution and an estimate of the outburst frequency of these new dwarf novae and those discovered by the Catalina Real-time Transient Survey (CRTS) indicates that besides systems that are faint because they are farther away, there also exists a population of intrinsically faint dwarf novae with rare outbursts.

  7. Experience with a high order programming language on the development of the Nova distributed control system

    Energy Technology Data Exchange (ETDEWEB)

    Suski, G.J.; Holloway, F.W.; Duffy, J.M.

    1983-05-10

    This paper explores the impact of an HOL on the development of the distributed computer control system for Nova laser fusion facility. As the world's most powerful glass laser, Nova will generate 150 trillion watt pulses of infrared light focused onto fusion targets a few millimeters in diameter. It will perform experiments designed to explore the feasibility of fusion as an energy source of the future. Nova will utilize fifty microcomputers and four VAX-11/780's in a distributed process control computer system architecture.

  8. SW Sex stars, old novae, and the evolution of cataclysmic variables

    CERN Document Server

    Schmidtobreick, Linda

    2014-01-01

    The population of cataclysmic variables with orbital periods right above the period gap are dominated by systems with extremely high mass transfer rates, the so-called SW Sextantis stars. On the other hand, some old novae in this period range which are expected to show high mass transfer rate instead show photometric and/or spectroscopic resemblance to low mass transfer systems like dwarf novae. We discuss them as candidates for so-called hibernating systems, CVs that changed their mass transfer behaviour due to a previously experienced nova outburst. This paper is designed to provide input for further research and discussion as the results as such are still very preliminary.

  9. Sintese e caracterização de novas quinazolinas polissubstituidas

    OpenAIRE

    Luis Fernando Cabeça

    2004-01-01

    Resumo: O presente trabalho teve como objetivo a obtenção de novas 4-anilinoquinazolinas polissubstituídas a partir de novos derivados do ácido antranílico. As primeiras rotas sintéticas testadas, partiram do ácido 3,4-diidroxibenzóico e do 4-metilcatecol, não levando a resultados satisfatórios. Sendo assim, uma nova rota sintética foi proposta partindo do 6-nitropiperonal, com um protetor diferente para as hidroxilas, o grupamento metilenodióxi. Com essa nova rota, em dois passos sintéticos ...

  10. Atmospheric deposition, operational report for air pollution 2003. NOVA 2003; Atmosfaerisk deposition, driftsrapport for Luftforurening i 2003 NOVA 2003

    Energy Technology Data Exchange (ETDEWEB)

    Ellermann, T.; Hertel, O.; Ambelas Skjoeth, C.; Kemp, K.; Monies, C.

    2004-12-01

    This report presents measurements and calculations from the atmospheric part of NOVA 2003 and covers results for 2003. It summarises the main results concerning concentrations and depositions of nitrogen, phosphorous and sulphur compounds related to eutrofication and acidification and selected heavy metals. Depositions of atmospheric compounds to Danish marine waters as well as land surface are presented. The measurements in the monitoring programme are supplemented with model calculations of concentrations and depositions of nitrogen and sulphur compounds to Danish land surfaces as well as marine waters, fjords and bays using the ACDEP model (Atmospheric Chemistry and Deposition). The model is a so-called trajectory model and simulates the physical and chemical processes in the atmosphere using meteorological and emission data input. (BA)

  11. Resultados econômicos da produção de cordeiros em confinamento utilizando na dieta casca de soja associada a quatro fontes de nitrogênio não-proteico Economic results of feedlot lamb using soybean husks associated with different non-protean nitrogen sources

    Directory of Open Access Journals (Sweden)

    Evâneo Alcides Ziguer

    2011-09-01

    Full Text Available O objetivo neste estudo foi avaliar o custo de produção e a resposta econômica da utilização de casca de soja (CS associada a duas fontes de nitrogênio não-proteico (NNP na terminação de cordeiros em confinamento. Foram utilizados 80 cordeiros mestiços Suffolk, com idade inicial de 69 ± 6 dias e peso vivo inicial de 23,11 ± 1,78 kg. Os animais foram distribuídos em quatro grupos, cada um com uma dieta formulada com uma fonte de NNP: grupo ureia convencional, na proporção de 1%; grupo ureia protegida, na proporção de 1%; grupo ureia protegida convencional, na proporção de 1% + 0,5% de ureia convencional, da dieta total, respectivamente; e grupo controle, sem fonte adicional de NNP. O custo total de produção do cordeiro até a desmama foi de R$ 85,27/animal. Entre os componentes desse custo, a categoria de ovelhas foi a principal contribuinte, com 68,55%, seguida pelos custos referentes ao próprio cordeiro (0-67 dias, que representaram 25,57%, e a dos carneiros, com participação de apenas 5,88%. O custo total médio da terminação em confinamento foi de R$ 57,73/cordeiro. O custo operacional efetivo (COEf representou R$ 57,35, ou 99,33% do custo total à terminação. As variáveis de maior representatividade do COEf foram alimentação (61,56% e impostos (31,06%. As dietas que permitiram obter margem bruta/cordeiro positiva foram aquelas com ureia convencional e sem fonte adicional de NNP (R$ 1,77 e R$ 4,35, respectivamente. No entanto, todas as dietas apresentaram margem líquida e resultado econômico negativos. Em sistemas de terminação de cordeiros em confinamento, o uso de dietas sem fonte adicional de nitrogênio não-proteico é a opção que permite obter melhor resultado zootécnico e econômico.The aim of this study was to evaluate the production costs and economic return of soybean husks (CS associated with two non-protein nitrogen (NNP sources, in feedlot finishing lamb. Eighty (80 Suffolk cross lambs

  12. Desempenho de cordeiros Santa Inês puros e cruzas Santa Inês com Texel, Ile de France e Bergamácia Performance of Santa Inês lambs and its crosses with Texel, Ile de France e Bergamacia lambs

    Directory of Open Access Journals (Sweden)

    Iraides Ferreira Furusho-Garcia

    2004-12-01

    Full Text Available O trabalho foi desenvolvido com o objetivo de estudar o efeito do sexo dos animais, do grupo genético e do peso de abate no desempenho de animais confinados. Foram utilizados 103 cordeiros, machos e fêmeas, Santa Inês puros (SS e cruzas Santa Inês com Texel (TS, Ile de France (FS e Bergamácia (BS, confinados em gaiolas individuais. Mediram-se a dieta fornecida e as sobras diárias, para cálculo do consumo de matéria seca (MS, energia metabolizável (EM, proteína digestível (PD e fibra em detergente neutro (FDN. Os cordeiros foram abatidos em quatro pesos: 15, 25, 35 e 45 kg de peso vivo. Avaliaram-se o ganho de peso diário (GPD, o número de dias no confinamento (ND, a conversão alimentar (CA e o consumo de MS, PD, EM e FDN, nas três fases de crescimento: 15 a 25 kg (1, 25 a 35 kg (2 e 35 a 45 kg (3. Também foram avaliados as idades de abate (IA, o peso do corpo vazio (PCVZ e rendimento de carcaça (RC. Aos 35 e 45 kg, os cordeiros TS e FS apresentaram IA inferiores e as cordeiras SS, IA superiores. O ND dos cordeiros BS de 35 a 45 kg foi maior que dos TS. Aos 35 e 45 kg, o PCVZ dos cordeiros TS e FS foram menores. Os melhores GPD foram dos cordeiros TS, seguidos do FS e SS. Os consumos de MS, PD, EM e FDN foram semelhantes entre os grupos genéticos, nas fases 1 e 2 de crescimento. Verificou-se que os cordeiros TS tenderam a aumentar o consumo, com o incremento de peso, enquanto os outros grupos tenderam a diminuir. A CA elevou-se com o aumento de peso, com exceção dos machos FS. Os machos não apresentaram diferenças na CA entre os grupos genéticos, entretanto, as fêmeas TS e FS apresentaram valores melhores. Aos 35 e 45 kg, as fêmeas apresentaram maiores RC que os machos. Aos 35 kg, os melhores RC foram dos machos TS.The work was carried out to evaluate the effect of animal sex, genetic group and slaugher weight on fedlot lambs performance. One hundred and three male and female lambs, purebred Santa Inês (SS and crosses

  13. Características de carcaça determinadas por ultrassonografia em tempo real e pós-abate de cordeiros terminados em confinamento com diferentes níveis de energia na dieta¹ Carcass traits determined by ultrasonography in real time and after slaughter of lambs finished in fedlot with diferent levels of energy in the diet

    Directory of Open Access Journals (Sweden)

    Felipe Queiroga Cartaxo

    2011-01-01

    Full Text Available Objetivou-se avaliar as características de carcaça por ultrassonografia em tempo real e após o abate e a relação entre essas características e os rendimentos de carcaça de cordeiros de diferentes genótipos terminados em confinamento com diversos níveis de energia na dieta. Foram utilizados 54 cordeiros não-castrados - 18 Santa Inês puros (SI, 18 ½Dorper x ½Santa Inês (Dp x SI e 18 ½Santa Inês x ½Sem Raça Definida (SI x SRD - com média de 150 dias de idade e peso médio de 22,60 kg no início do experimento. As dietas continham 17% de proteína bruta e 2,40 Mcal/kg MS e 2,90 Mcal/kg MS. As mensurações realizadas por ultrassonografia e diretamente na carcaça dos cordeiros apresentaram resultados similares. Os cordeiros alimentados com a dieta contendo 2,90 Mcal/kg apresentaram maior área de olho-de-lombo, melhor conformação e acabamento de carcaça e maior quantidade de gordura pélvico-renal. Os cordeiros Dp x SI apresentaram maior área de olho-de-lombo e musculosidade por 100 kg de PV em comparação aos SI x SRD e foram superiores a todos os genótipos quanto à espessura de gordura subcutânea, à conformação e ao acabamento de carcaça. O marmoreio observado nos cordeiros Dp x SI foi superior aos dos Santa Inês. As correlações das medidas tomadas por ultrassonografia e na carcaça foram altas e significativas, exceto o marmoreio. Houve correlação significativa entre conformação da carcaça e acabamento, marmoreio, espessura de gordura subcutânea e gordura pélvico-renal. As gorduras de cobertura avaliadas subjetivamente e objetivamente apresentaram correlações altas e significativas. A dieta e o genótipo influenciam as características de carcaça de cordeiros.The objective of this study was to evaluate carcass traits through ultrasonography in real time and after slaughter and the relationship between these traits and carcass yields of lambs with different genotypes finished in feedlot with several

  14. Rendimento dos componentes não-carcaça de cordeiros alimentados com silagem de milho ou cana-de-açúcar e dois níveis de concentrado Non-carcass components yield of lambs fed corn silage or sugar cane under two levels of concentrate

    Directory of Open Access Journals (Sweden)

    Greicy Mitzi Bezerra Moreno

    2011-12-01

    Full Text Available Objetivou-se avaliar o rendimento dos componentes não-carcaça de cordeiros terminados em confinamento recebendo dietas formuladas com silagem de milho ou cana-de-açúcar e dois níveis de concentrado. Utilizaram-se 32 cordeiros Ile de France, não-castrados, alimentados com silagem de milho ou cana-de-açúcar em duas relações volumoso:concentrado, 60:40 ou 40:60. Os cordeiros foram mantidos em confinamento até atingirem 32 kg de peso corporal (PCA, quando foram abatidos. Após a sangria, todos os constituintes não-carcaça (sangue, pele, cabeça, patas, rúmen, retículo, omaso, abomaso, intestino delgado, intestino grosso, baço, fígado, coração, pulmão com traqueia, pâncreas, rins com gordura perirrenal, gorduras omental e mesentérica foram separados e pesados, calculando-se suas porcentagens em relação ao PCA. O conteúdo do trato gastrintestinal (TGI foi maior nos cordeiros alimentados com cana-de-açúcar (15,17% e 60% de volumoso (14,55%; enquanto as gorduras omental e perirrenal foram maiores nos cordeiros que receberam silagem de milho, 0,53 e 0,63%, respectivamente. A relação volumoso:concentrado e o tipo de volumoso afetaram as proporções de rúmen, omaso e intestino delgado em relação ao peso total do trato gastrintestinal. A relação volumoso:concentrado e o tipo de volumoso influenciam o conteúdo do trato gastrintestinal de cordeiros, afetando indiretamente os rendimentos de carcaça. O tipo de alimentação tem maior influência sobre as proporções dos órgãos responsáveis pela digestão e absorção de nutrientes. Os fatores que influenciam os componentes não-carcaça de cordeiros são variados e contraditórios, o que torna necessária a realização de mais pesquisas para incentivar sua utilização e, consequentemente, agregar valor aos sistemas de produção de carne ovina.The objective of this result was to evaluate the yields of non-carcass components of lambs finished in feedlot feeding on diets

  15. Effect of breed type and ionophore supplementation on growth and carcass characteristic in feedlot hair lambs Efeito do grupo genético e da suplementação com ionóforos sobre o crescimento e as características de carcaça de cordeiros deslanados confinados

    Directory of Open Access Journals (Sweden)

    Jaime Salinas-Chavira

    2010-03-01

    Full Text Available The effects of supplementing feedlot diets with ionophores and breed type were assessed on growth rate and carcass characteristics in hair lambs. Twenty four intact males, 12 Pelibuey × Dorper (PDo and 12 Pelibuey × Damara (PDa lambs, 17.9 ± 3.7 kg initial weight, were housed in individual pens for a 60-d feeding trial. The lambs were assigned randomly into four diets: control without additives (C; 25 µg/g monensin (M; 28 µg/g salinomycin (S; 28 µg/g S for 20 d, and 25 µg/g M for the next 40 d (SM. Each diet was supplied to six lambs. Data were analyzed as a randomized complete block design in a 4 × 2 factorial arrangement, with four diets and two breed types of hair lambs (PDo and PDa. All diets were formulated to contain 14% CP and 2.6 Mcal ME/kg dry matter. At the end of the feeding trial carcass images were recorded in the last intercostal space (12th and 13th ribs using ultrasound equipment to measure the Longissimus dorsi muscle area and subcutaneous fat (SF. The average daily gain (ADG, daily dry matter intake, feed:gain ratio, subcutaneous fat and Longissimus dorsi area were not affected by ionophore supplementation.. The Pelibuey × Dorper group tended to show better average daily gain than Pelibuey × Damara (262 g/d and 235 g/d, respectively. Daily dry matter intake, feed:gain ratio and subcutaneous fat were not affected by breed type. The Pelibuey × Dorper lambs had greater Longissimus dorsi area (16.74 cm² than the Pelibuey × Damara (14.29 cm² lambs. The growth rate was not influenced by the inclusion of ionophores. Pelibuey × Dorper lambs showed better average daily gain and carcass characteristics than Pelibuey × Damara lambs.Avaliaram-se os efeitos da suplementação de dietas de confinamento com ionóforos e da raça do animal na taxa de crescimento e nas características de carcaça de cordeiros deslanados. Vinte e quatro machos não-castrados – 12 cordeiros Pelibuey × Dorper (PDo e 12 cordeiros Pelibuey

  16. Observations and Analysis of the GK Persei Nova Shell and its "Jet-like" Feature

    CERN Document Server

    Harvey, E; Boumis, P; Akras, S

    2016-01-01

    GK Persei (1901, the 'Firework Nebula') is an old but bright nova remnant that offers a chance to probe the physics and kinematics of nova shells. The kinematics in new and archival longslit optical echelle spectra were analysed using the shape software. New imaging from the Aristarchos telescope continues to track the proper motion, extinction and structural evolution of the knots, which have been observed intermittently over several decades. We present for the first time, kinematical constraints on a large faint 'jet' feature, that was previously detected beyond the shell boundary. These observational constraints allow for the generation of models for individual knots, interactions within knot complexes, and the 'jet' feature. Put together, and taking into account dwarf-nova accelerated winds emanating from the central source, these data and models give a deeper insight into the GK Per nova remnant as a whole.

  17. A Method for Telluric Line Removal from Supernova and Nova Spectra

    Science.gov (United States)

    Jack, D.

    2017-04-01

    We present a new method for removing telluric lines from high resolution supernova and nova spectra. This simple and quick method has the advantage of also eliminating any interstellar and intergalactic absorption features, and it smoothens the spectra removing noise and any possible cosmic-ray hits. The method identifies narrow lines in the very broad features of supernova and nova spectra and removes all of them. We applied the method to observed high resolution (R≍20,000) spectra of the type Ia supernova SN 2014J and performed a study of the effects of telluric lines in low resolution spectra of this supernova. The differences in flux can be around 25% in some wavelength ranges with broad telluric bands. In addition, we demonstrate that this method can also be applied to high resolution spectra of novae and present as an example the telluric line removal in the spectra of Nova V5668 Sgr.

  18. Early optical spectra of nova V1369 Cen show presence of Lithium

    CERN Document Server

    Izzo, L; Mason, E; Matteucci, F; Romano, D; Pasquini, L; Vanzi, L; Jordan, A; Fernandez, J M; Bluhm, P; Brahm, R; Espinoza, N; Williams, R

    2015-01-01

    We present early high resolution spectroscopic observations of the nova V1369 Cen. We have detected an absorption feature at 6695.6 \\AA\\, that we have identified as blue--shifted $^7$Li I $\\lambda$6708 \\AA. The absorption line, moving at -550 km/s, was observed in five high-resolution spectra of the nova obtained at different epochs. On the basis of the intensity of this absorption line we infer that a single nova outburst can inject in the Galaxy $M_{Li} =$ 0.3 - 4.8 $\\times 10^{-10}$ M$_{\\odot}$. Given the current estimates of Galactic nova rate, this amount is sufficient to explain the puzzling origin of the overabundance of Lithium observed in young star populations.

  19. NOVAS TECNOLOGIAS E FORMAÇÃO DE PROFESSORES DO CAMPO: PARCERIAS EM DEBATE

    OpenAIRE

    2013-01-01

    O presente artigo enfoca as mediações das Novas Tecnologias (NT) na formação de professores da modalidade Educação a Distância (EAD) na Universidade Federal do Espírito Santo. A investigação parte de questionamentos sobre as mediações das Novas Tecnologias na formação docente em escolas do campo. A pesquisa permite identificar novas tendências teórico-metodológicas, mediadas por espaços interativos produzidos a partir da introdução de novas tecnologias no processo de ensino na modalidade a di...

  20. Fermi Establishes Classical Novae as a Distinct Class of Gamma-ray Sources

    Science.gov (United States)

    Ackermann, M.; Ajello, M.; Albert, A.; Baldini, L.; Ballet, J.; Bastieri, D.; Bellazzini, R.; Bissaldi, E.; Blandford, R. D.; Bloom, E. D.; Bottacini, E.; Brandt, T. J.; Bregeon, J.; Bruel, P.; Buehler, R.; Buson, S.; Caliandro, G. A.; Cameron, R. A.; Caragiulo, M.; Caraveo, P. A.; Ferrara, E. C.; Harding, A. K.; Hays, E.; Perkins, J. S.; Thompson, D. J.

    2014-01-01

    A classical nova results from runaway thermonuclear explosions on the surface of a white dwarf that accretes matter from a low-mass main-sequence stellar companion. In 2012 and 2013, three novae were detected in gamma rays and stood in contrast to the first gamma-ray detected nova V407 Cygni 2010, which belongs to a rare class of symbiotic binary systems. Despite likely differences in the compositions and masses of their white dwarf progenitors, the three classical novae are similarly characterized as soft spectrum transient gamma-ray sources detected over 2-3 week durations. The gamma-ray detections point to unexpected high-energy particle acceleration processes linked to the mass ejection from thermonuclear explosions in an unanticipated class of Galactic gamma-ray sources.

  1. Formation of Novae and Coronae on Venus. Tectonophysical Modeling Using Gravity Models

    Science.gov (United States)

    Krassilnikov, A. S.

    2001-03-01

    Novae and coronae formation was simulated using caoutchouc as a model of lower ductile part of lithosphere and dry flour as a model of upper brittle part of it. Distribution and character of the deformational structures is described.

  2. Influência da castração e da idade de abate sobre as características subjetivas e instrumentais da carne de cordeiros Corriedale Effects of castration and slaughtering age on the subjective and instrumental characteristics of meat from Corriedale lambs

    Directory of Open Access Journals (Sweden)

    Eunice de Leon Rota

    2006-12-01

    Full Text Available Este trabalho foi realizado com o objetivo de avaliar o efeito da castração e da idade de abate sobre as características subjetivas e instrumentais da carne de cordeiros Corriedale criados em condições extensivas de pastagem natural. Foram utilizados 60 cordeiros machos (30 não-castrados e 30 castrados abatidos no ano de 2003, aos 120, 210 e 360 dias de idade, nos meses de fevereiro, maio e outubro, respectivamente. As avaliações da carne foram realizadas no músculo Longissimus dorsi. Pela análise da variância, verificou-se que não houve efeito da interação castração × idade de abate nas características estudadas. Foi encontrada significância para a idade de abate nas características subjetivas espessura de gordura de cobertura e marmoreio (os índices foram mais baixos nos animais mais velhos e em todas as características instrumentais avaliadas, principalmente maciez, que diminuiu com o aumento da idade de abate. O efeito da castração foi significativo somente no componente de cor L*. A qualidade da carne foi similar entre cordeiros Corriedale castrados e não-castrados criados extensivamente em pastagem natural, entretanto, a idade de abate influenciou a qualidade da carne, que foi melhor nos animais abatidos aos 120 dias.The objective of this trial was to evaluate the effects of castration and slaughtering age on subjective and instrumental characteristics of meat from Corriedale lambs raised on native pasture. Sixty male lambs (30 castrated and 30 intact slaughtered at 120, 210 and 360 days of age were used in this experiment. The Longissimus dorsi muscle was used for all meat evaluations and analysis. No significant castration × slaughtering age interaction was observed for the studied variables. A significant slaughtering age effect was found for meat fat thickness and marbling, which had lower scores in animals slaughtered at more advanced age as well as for all instrumental characteristics of the meat, mainly

  3. Efeito do nível de energia metabolizável na composição dos tecidos da carcaça de cordeiros da raça Santa Inês Effect of metabolizable energy level on the carcass tissues composition of Santa Ines lambs

    Directory of Open Access Journals (Sweden)

    T.R.V. Almeida

    2009-12-01

    Full Text Available Estudou-se a influência da energia metabolizável (EM, pela inclusão de percentuais crescentes de fibra em detergente neutro (FDNf, proveniente de forragem, sobre a composição dos tecidos da carcaça de 64 cordeiros Santa Inês. Os tratamentos (dietas foram: dieta A - com 8,7% de FDNf; dieta B - com 17,3%; dieta C - com 26,0% e dieta D - com 34,7% de FDNf na dieta. Quatro animais de cada tratamento foram abatidos aos 43, 83, 123 e 173 dias. Os cordeiros que receberam as dietas A e B apresentaram maiores pesos dos tecidos ósseo (TO, muscular (TM, adiposo (TA e outros (OT na carcaça fria, a partir dos 83 dias de idade. O rendimento de TO na carcaça fria dos animais que receberam as dietas A e B foi menor, enquanto as proporções de TA foram maiores a partir dos 83 dias de idade. A regressão de cada variável, em função do consumo de EM total (Mcal, para cada tratamento, mostrou que a deposição de TA em cordeiros alimentados com a dieta A foi mais intensa.The effect of metabolizable energy level (ME, due to increasing levels of forage nitrogen detergent fiber (fNGF, on the carcass tecidual composition of 64 Santa Inês lambs was evaluated. Four treatments (diets were: diet A- fNDF; diet B- 17.3%; of fNDF; diet C- 26.0% of fNDF; and diet D- 34.7% of 8.7% fNDF in the diet. Four animals of each treatment were slaughtered at 43, 83, 123, and 173 days. Lambs fed diets A and B, showed higher weight of bonne tissue (BT, muscular tissue (MT, fatty tissue (FT, and other tissues (OT in cold carcass at 83 days of age. The percentage of BT in cold carcass of the lambs fed diets A and B was lower, and percentage of FT was higher, after 83 days of age. The regression of each variable on ME total intake (Mcal, for each treatment, suggested higher intensity of deposition of FT for lambs fed diet A.

  4. Discovery of ten galactic Nova candidates in the VVV disk area

    Science.gov (United States)

    Saito, R. K.; Minniti, D.; Catelan, M.; Angeloni, R.; Beamin, J. C.; Palma, T.; Gutierrez, L. A.; Montenegro, K.

    2016-01-01

    We report the discovery of ten likely Galactic novae by the VVV Survey in its disk area (vvvsurvey.org; Minniti et al. 2010, New Astronomy, 15, 433). A search for high-amplitude transients on the VVV disk data taken during the 2010-2013 seasons detected the presence of ten stellar sources fading in brightness by at least Delta_Ks=3 mag with their light curves following the expected behavior of a nova outburst.

  5. A arbitragem internacional e a nova lei paraguaia de contratos internacionais

    Directory of Open Access Journals (Sweden)

    José Antonio Moreno Rodríguez

    2016-05-01

    Full Text Available O Paraguai começa o ano de 2015 com uma nova lei de contratos internacionais, em consonância com as propostas vanguardistas avançadas por prestigiosas organizações codificadoras do mundo e das Américas. Nesta contribuição, se apresenta e explica a nova lei paraguaia no contexto, expondo suas potencialidades com respeito à arbitragem internacional.

  6. Shell and explosive hydrogen burning. Nuclear reaction rates for hydrogen burning in RGB, AGB and Novae

    Energy Technology Data Exchange (ETDEWEB)

    Boeltzig, A. [Gran Sasso Science Institute, L' Aquila (Italy); Bruno, C.G.; Davinson, T. [University of Edinburgh, SUPA, School of Physics and Astronomy, Edinburgh (United Kingdom); Cavanna, F.; Ferraro, F. [Dipartimento di Fisica, Universita di Genova (Italy); INFN, Genova (Italy); Cristallo, S. [Osservatorio Astronomico di Collurania, INAF, Teramo (Italy); INFN, Napoli (Italy); Depalo, R. [Dipartimento di Fisica e Astronomia, Universita di Padova, Padova (Italy); INFN, Padova (Italy); DeBoer, R.J.; Wiescher, M. [University of Notre Dame, Institute for Structure and Nuclear Astrophysics, Joint Institute for Nuclear Astrophysics, Notre Dame, Indiana (United States); Di Leva, A.; Imbriani, G. [Dipartimento di Fisica, Universita di Napoli Federico II, Napoli (Italy); INFN, Napoli (Italy); Marigo, P. [Dipartimento di Fisica e Astronomia, Universita di Padova, Padova (Italy); Terrasi, F. [Dipartimento di Matematica e Fisica Seconda Universita di Napoli, Caserta (Italy); INFN, Napoli (Italy)

    2016-04-15

    The nucleosynthesis of light elements, from helium up to silicon, mainly occurs in Red Giant and Asymptotic Giant Branch stars and Novae. The relative abundances of the synthesized nuclides critically depend on the rates of the nuclear processes involved, often through non-trivial reaction chains, combined with complex mixing mechanisms. In this paper, we summarize the contributions made by LUNA experiments in furthering our understanding of nuclear reaction rates necessary for modeling nucleosynthesis in AGB stars and Novae explosions. (orig.)

  7. Strategies of design, development and activation of the Nova control system

    Energy Technology Data Exchange (ETDEWEB)

    Holloway, F.W.

    1983-06-30

    Nova and Novette are large complex experimental laser facilities which require extensive and sophisticated control systems for their successful operation. Often, in major controls projects, certain invisible aspects of the project, such as overall strategy, management, resources and historical constraints, have a more profound effect upon success than any specific hardware/software design. The design and performance of the Nova/Novette laser control system will be presented with special emphasis upon these often controversial aspects.

  8. The evolution of a large laser control system - From Shiva to Nova

    Energy Technology Data Exchange (ETDEWEB)

    Suski, G.J.; Holloway, F.W.

    1979-09-01

    The Nova laser system is a 200 terawatt laser facility under construction at Lawrence Livermore Laboratory. Its current operational predecessor, the 30 terawatt Shiva laser, is controlled and diagnosed via a network of 50 computers. Although the highly distributed Shiva control system has proven effective and reliable, the need for more integrated process control on Nova is leading to a more centralized architecture. An overview of these control systems is presented and their differences are discussed.

  9. Uma padre na aldeia global : nova evangelização e novas tecnologias de informação e comunicação

    OpenAIRE

    Aguiar, Américo Manuel Alves

    2012-01-01

    Nesta dissertação, revemos os últimos cem anos de pronunciamentos dos sucessores de Pedro, do Papa Leão XIII, ao Papa Bento XVI, atestando a atenção e interesse com que a igreja católica sempre olhou para as potencialidades oferecidas pelas novas tecnologias de informação e de comunicação. Olhamos de um ponto de vista comunicacional para a urgência da Nova Evangelização pronunciada pelo Papa João Paulo II, dando continuidade ao já expresso pelo Papa Paulo VI e pelo próprio II ...

  10. V5852 Sgr: An Unusual Nova Possibly Associated with the Sagittarius Stream

    CERN Document Server

    Aydi, E; Whitelock, P A; Mohamed, S; Wyrzykowski, Ł; Udalski, A; Vaisanen, P; Nagayama, T; Dominik, M; Scholz, A; Onozato, H; Williams, R E; Hodgkin, S T; Nishiyama, S; Yamagishi, M; Smith, A M S; Ryu, T; Iwamatsu, A; Kawamata, I

    2016-01-01

    We report spectroscopic and photometric follow-up of the peculiar nova V5852~Sgr (discovered as OGLE-2015-NOVA-01), which exhibits a combination of features from different nova classes. The photometry shows a flat-topped light curve with quasi-periodic oscillations, then a smooth decline followed by two fainter recoveries in brightness. Spectroscopy with the Southern African Large Telescope shows first a classical nova with an Fe II or Fe IIb spectral type. In the later spectrum, broad emissions from helium, nitrogen and oxygen are prominent and the iron has faded which could be an indication to the start of the nebular phase. The line widths suggest ejection velocities around $1000\\,{\\rm km\\,s^{-1}}$. The nova is in the direction of the Galactic bulge and is heavily reddened by an uncertain amount. The $V$ magnitude 16 days after maximum enables a distance to be estimated and this suggests that the nova may be in the extreme trailing stream of the Sagittarius dwarf spheroidal galaxy. If so it is the first no...

  11. Pulsed power supply for Nova Upgrade. Final report, August 1, 1991 to March 31, 1992

    Energy Technology Data Exchange (ETDEWEB)

    Bacon, J.L.; Kajs, J.P.; Walls, A.; Weldon, W.F.; Zowarka, R.C. [Univ. of Texas, Austin, TX (US). Center for Electromechanics

    1992-12-31

    This report describes work carried out at the Center for Electromechanics at The University of Texas at Austin (CEM-UT). A baseline design of the Nova Upgrade has been completed by Lawrence Livermore National Laboratory. The Nova Upgrade is an 18 beamline Nd: glass laser design utilizing fully relayed 4x4 30 cm aperture segmented optical components. The laser thus consists of 288 independent beamlets nominally producing 1.5 to 2.0 MJ of 0.35 {mu}m light in a 3 to 5 ns pulse. The laser design is extremely flexible and will allow a wide range of pulses to irradiate ICF targets. This facility will demonstrate ignition/gain and the scientific feasibility of ICF for energy and defense applications. The pulsed power requirements for the Nova Upgrade are given. CEM-UT was contracted to study and develop a design for a homopolar generator/inductor (HPG/inductor) opening switch system which would satisfy the pulsed power supply requirements of the Nova Upgrade. The Nd:glass laser amplifiers used in the Nova Upgrade will be powered by light from xenon flashlamps. The pulsed power supply for the Nova Upgrade powers the xenon flashlamps. This design and study was for a power supply to drive flashlamps.

  12. Binary orbits as the driver of gamma-ray emission and mass ejection in classical novae

    CERN Document Server

    Chomiuk, Laura; Yang, Jun; O'Brien, T J; Paragi, Zsolt; Mioduszewski, Amy J; Beswick, R J; Cheung, C C; Mukai, Koji; Nelson, Thomas; Ribeiro, Valerio A R M; Rupen, Michael P; Sokoloski, J L; Weston, Jennifer; Zheng, Yong; Bode, Michael F; Eyres, Stewart; Roy, Nirupam; Taylor, Gregory B

    2014-01-01

    Classical novae are the most common astrophysical thermonuclear explosions, occurring on the surfaces of white dwarf stars accreting gas from companions in binary star systems. Novae typically expel ~10^(-4) solar masses of material at velocities exceeding 1,000 kilometres per second. However, the mechanism of mass ejection in novae is poorly understood, and could be dominated by the impulsive flash of thermonuclear energy, prolonged optically thick winds, or binary interaction with the nova envelope. Classical novae are now routinely detected in gigaelectronvolt gamma-ray wavelengths, suggesting that relativistic particles are accelerated by strong shocks in the ejecta. Here we report high-resolution radio imaging of the gamma-ray-emitting nova V959 Mon. We find that its ejecta were shaped by the motion of the binary system: some gas was expelled rapidly along the poles as a wind from the white dwarf, while denser material drifted out along the equatorial plane, propelled by orbital motion. At the interface ...

  13. The Contribution of Chemical Abundances in Nova Ejecta to the Interstellar Medium

    CERN Document Server

    Li, Fanger; Lu, Guoliang; Wang, Zhaojun

    2016-01-01

    According to the nova model from \\citet{Yaron2005} and \\citet{Jose1998} and using Monte Carlo simulation method, we investigate the contribution of chemical abundances in nova ejecta to the interstellar medium (ISM) of the Galaxy. We find that the ejected mass by classical novae (CNe) is about $2.7\\times10^{-3}$ $ \\rm M_\\odot\\ {\\rm yr^{-1}}$. In the nova ejecta, the isotopic ratios of C, N and O, that is, $^{13}$C/$^{12}$C, $^{15}$N/$^{14}$N and $^{17}$O/$^{16}$O, are higher about one order of magnitude than those in red giants. We estimate that about 10$\\%$, 5$\\%$ and 20$\\%$ of $^{13}$C, $^{15}$N and $^{17}$O in the ISM of the Galaxy come from nova ejecta, respectively. However, the chemical abundances of C, N and O calculated by our model can not cover all of observational values. This means that there is still a long way to go for understanding novae.

  14. 97-ERD-022 final report: Supernova on Nova

    Energy Technology Data Exchange (ETDEWEB)

    Remington, B A

    1999-03-11

    This is the final year of the 3-year LDRD-ERD involving Lasers, D&NT, Physics, and ILSA to develope astrophysics experiments on intense lasers such as the Nova and Gekko lasers. During this 3 year period, we have developed a highly successful experiment probing the hydrodynamics of the explosion phase of core-collapse supernovae, which occurs during the first ~3 hours after core collapse. This was in collaboration with the Univ. of Arizona and CEA/Saclay. We also developed a very successful experiment to probe the hydrodynamics of the later time, young remnant phase, meaning the first ~10-20 years after core collapse. This was in collaboration with the Univ. of Michigan and Univ. of Colorado. Finally, we developed during the final year an exquisite experiment to probe the dynamics of radiative, high Mach number astrophysical jets, in collaboration with the Univ. of Maryland and Osaka Univ. Each experiment has received very high visibility, with a multitude of publications, both in the technical journals (most importantly, the astrophysical journals) and in the popular press. The attached publication list shows 25 papers published or submitted to technical journals, 5 articles appearing in the popular press (including a cover story of Sky and Telescope), and 65 conference presentations, ~10 of which were invited talks. The most important papers to come out of this effort was a comprehensive theory paper for Ap. J. establishing the rigorous scaling between laboratory laser experiments and the astrophysical subjects of interest: supernovae, supernova remnants, and jets; and a review article for Science covering this emerging subfield of Astrophysics on Intense Lasers. Since there are so many publications that have resulted from this LDRD project, only these two most important papers are attached. The rest are properly referenced, and can be found online or in the library. In anticipation of the closing of the Nova laser, we have successfully proposed transferring the

  15. Avaliação epidemiológica, clínica, anatomopatológica e etiológica de surtos de ataxia em cabritos e cordeiros

    Directory of Open Access Journals (Sweden)

    Santos Néria Vania Marcos dos

    2006-01-01

    Full Text Available Nos anos de 2001 e 2002, 46 cabritos (CAB e 35 cordeiros (COR de uma propriedade do agreste do Estado de Pernambuco foram acometidos por ataxia enzoótica (AE de forma tardia. Houve aumento da incidência do 1o ano (46,3% - CAB; 24,2% COR para o ano subseqüente (100% - CAB e COR. Somente no ano de 2001, houve maior incidência em CAB (P<0,002 que nos COR. Todos os animais acometidos sucumbiram, com exceção de um CAB e um de COR. O quadro clínico variou de acordo com a idade em que surgiram os sintomas, ou seja, de 30 a 45 dias os animais manifestaram paralisia dos membros anteriores e posteriores, acompanhada de espasticidade muscular e morte; com mais de 45 dias, ocorreu paralisia flácida ou espástica apenas dos membros posteriores e morte; somente os cabritos com menos de 45 dias apresentaram movimentos verticais de cabeça. As lesões histopatológicas evidenciadas foram: degeneração axonal, esferóides, gliose e dismielinização no segmento ventral e lateral da medula espinhal. Nos animais com menos de 45 dias, essas lesões foram evidentes na região cervical e nos animas mais velhos na região lombar. Apenas nos cabritos foi constatada lesão degenerativa no cerebelo. A dieta oferecida ao rebanho continha quantidades adequadas de cobre, porém os animais acometidos por AE apresentaram baixos teores de cobre no fígado (45,8mg kg-1 MS. Os elementos antagonizantes do cobre, Mo, S, e Zn, estavam normais, com exceção do ferro, que estava em alta concentração tanto no solo (8600mg kg-1 quanto nos alimentos (284mg kg-1. O excesso de ingestão de ferro sugere ter provocado a carência de cobre nos animais.

  16. High resolution geomagnetic field observations at Terra Nova bay, Antarctica

    Directory of Open Access Journals (Sweden)

    P. Palangio

    1996-06-01

    Full Text Available he preliminary results obtained from the analysis in the micropulsation frequency range of high time resolution magnetic field data recorded at the Antarctic Italian geomagnetic observatory at Terra Nova Bay for 11 consecutive days in February 1994 are reported. The spectral index over the whole Pcl-Pc5 frequency range is of the order of 3.5 and its value significantly increases beyond about 50 mHz. Spectral peaks in the Pc3 frequency range are common, especially during the daytime hours, and are probably due to the direct penetration of upstream waves in the cusp region. From the local time distribution of the micro pulsation power, a signifi - cant activity enhancement around the local magnetic noon emerges, in agreement with previous observations. The analysis of the signal polarisation characteristics in the horizontal plane shows a predominant CW polarisation in the Pcl-Pc3 frequency ranges with the major axis of the polarisation ellipse in the first quadrant.

  17. Evolution of the accretion flow in Nova Muscae 1991

    CERN Document Server

    Zycki, P T; Smith, D; Zycki, Piotr; Done, Chris; Smith, David

    1998-01-01

    We identify the X-Ray reflected component in the Ginga spectra of Nova Muscae 1991, a Black Hole transient system used as the prototype for the recent model of Esin, McClintock & Narayan (1997) based on advection dominated disk solutions. We see that the reflected spectrum is generally significantly relativistically smeared, and use this, together with the amplitude of reflection, to track the innermost extent of the accretion disk. The optically thick disk switches from being highly ionized to nearly neutral during the transition from high to low state, and the inner radius of the disk moves outwards during the low state decline. Qualitatively, this overall trend is compatible with Esin et al.'s model, but quantitatively, the retreat of the inner disk during the high to low state transition is much slower than predicted. The hard (low state) spectra are not produced solely by an optically thin accretion flow: optically thick material within 20-100 Rg is generally present.

  18. Ano Novo: novas conquistas, novos desafios e um mesmo compromisso

    Directory of Open Access Journals (Sweden)

    André Luís Gemal

    2014-02-01

    Full Text Available Neste mês de fevereiro de 2014 lançamos o primeiro número do nosso segundo volume, mantendo assim o cronograma programado e a periodicidade proposta para nossa revista Vigilância Sanitária em Debate: Sociedade, Ciência & Tecnologia. Após sua inserção no sistema Qualis, da Capes, ao final do ano passado, iniciamos 2014 com novas e importantes conquistas, entre elas, a inclusão na base de dados do Latindex e a nossa participação no sistema de classificação DOI. Neste segundo ano de vida da Vigilância Sanitária em Debate permanecemos com o mesmo compromisso de estimular a divulgação de saberes da área que, por vezes, estiveram sem espaço apropriado em veículos de divulgação reconhecidos no campo da saúde pública. O corpo editorial toma essa perspectiva como um desafio constante de nossa revista.

  19. Em busca de novas estratégias de desenvolvimento

    Directory of Open Access Journals (Sweden)

    Ignacy Sachs

    1995-12-01

    Full Text Available Na véspera da Conferência sobre desenvolvimento social em Copenhague (1995, o autor defende novas estratégias condizentes com uma axiologia do desenvolvimento. Para ele, não há desenvolvimento sem crescimento equilibrado dentro de cada país e nas relações Norte-Sul. Por outro lado, não se pode prescindir da ecologia. Finalmente o objetivo do desenvolvimento é o homem, sua cultura própria, seus valores universais: o direito à inserção produtiva e à participação enquanto cidadão, o que supõe um Estado democrático, regulador de uma economia mista. No plano jurídico, o autor sugere a criação de um foro internacional independente.On the eve of the International Social Conference in Copenhagen (1995, the author defends new strategies, suitable for a development axiology. According to him, there is no development without a balanced growth within each country and in the North-South relations. On the other hand, one cannot ignore ecology. Finally, the target of development is man, his own culture, his universal values: the right to a productive insertion and to the participation as a citizen. This pressuposes a democratic State, regulator of a mixed economy. At the juridic level, the author suggests the creation of an independent international forum.

  20. NSV 1907 - A new eclipsing, nova-like cataclysmic variable

    Science.gov (United States)

    Hümmerich, Stefan; Gröbel, Rainer; Hambsch, Franz-Josef; Dubois, Franky; Ashley, Richard; Gänsicke, Boris T.; Vanaverbeke, Siegfried; Bernhard, Klaus; Wils, Patrick

    2017-01-01

    NSV 1907, formerly listed as an irregular variable in variability catalogues, was classified as an Algol-type eclipsing binary in the Catalina Surveys Periodic Variable Star Catalogue. We have identified NSV 1907 as an ultraviolet (UV) bright source using measurements from the GALEX space telescope and detected obvious out-of-eclipse variability in archival photometric data from the Catalina Sky Survey, which instigated a closer examination of the object. A spectrum and extensive multicolour photometric observations were acquired, from which we deduce that NSV 1907 is a deeply eclipsing, nova-like cataclysmic variable. Apart from the orbital variations (deep eclipses with a period of P ≈ 6.63 hours), changes in mean brightness and irregular short-term variability (flickering) were observed. The presence of a secondary minimum at phase φ ≈ 0.5 was established, which indicates a significant contribution of the companion star to the optical flux of the system. We find possible evidence for sinusoidal variations with a period of P ≈ 4.2 d, which we interpret as the nodal precession period of the accretion disc. No outbursts or VY Scl-like drops in brightness were detected either by the CSS or during our photometric monitoring. Because of its spectral characteristics and the observed variability pattern, we propose NSV 1907 as a new moderately bright long-period SW Sextantis star. Further photometric and spectroscopic observations are encouraged.

  1. Abundance analysis of the recurrent nova RS Ophiuchi (2006 outburst)

    CERN Document Server

    Das, Ramkrishna

    2015-01-01

    We present an analysis of elemental abundances of ejecta of the recurrent nova RS Oph using published optical and near-infrared spectra during the 2006 outburst. We use the CLOUDY photoionization code to generate synthetic spectra by varying several parameters, the model generated spectra are then matched with the observed emission line spectra obtained at two epochs. We obtain the best fit model parameters through the $\\chi^{2}$ minimization technique. Our model results fit well with observed optical and near-infrared spectra. The best-fit model parameters are compatible with a hot white dwarf source with T$_{BB}$ of 5.5 - 5.8 $\\times$ 10$^{5}$ K and roughly constant a luminosity of 6 - 8 $\\times$ 10$^{36}$ ergs s$^{-1}$. From the analysis we find the following abundances (by number) of elements with respect to solar: He/H = 1.8 $\\pm$ 0.1, N/H = 12.0 $\\pm$ 1.0, O/H = 1.0 $\\pm$ 0.4, Ne/H = 1.5 $\\pm$ 0.1, Si/H = 0.4 $\\pm$ 0.1, Fe/H = 3.2 $\\pm$ 0.2, Ar/H = 5.1 $\\pm$ 0.1, and Al/H = 1.0 $\\pm$ 0.1, all other elem...

  2. GK Per 2015 dwarf nova covered by Suzaku

    CERN Document Server

    Yuasa, Takayuki; Ishida, Manabu

    2016-01-01

    The intermediate polar GK Per exhibited a dwarf nova outburst in March-April 2015. Suzaku X-ray telescope serendipitously captured the onset of the outburst during its pre-scheduled pointing observation spanning four days. In this paper, we present temporal and spectral analysis results of this outburst, together with those from archival data of quiescent obtained in 2009 and 2014. Our temporal analysis confirmed previously reported spin modulation of X-ray count rates in outburst with a WD spin period of P_WD=351.4+/-0.5 s. The modulation is also detected in the hard X-ray band (16-60 keV), and spectral modeling of the absorption suggests obscuration by a dense absorption with a line-of-sight column density of N_H>10^23 cm^-2. A complex time evolution of spin modulation profiles is seen; the spin minimum phase shifts from phase ~0.25 in the first half of the observation to ~0.65 in the second one, and the pulse shape significantly changes epoch by epoch. Spectral fitting in the Fe Kalpha band revealed an inc...

  3. Abundance analysis of the slow nova PW Vulpeculae 1984

    CERN Document Server

    Schwarz, G J; Shore, S N; Hauschildt, P H; Schwarz, Greg J.; Shore, Steven N.; Hauschildt, Peter H.

    1997-01-01

    We determine the elemental abundances for the ejecta of the slow nova PW Vul 1984. Our technique uses a minimization of the emission line fits of a photoionization model to available ultraviolet, optical and infrared spectra. We find the following abundances (by number) with respect to solar: He/H = 1.0 $^{+7}_{-2}$. In addition, there is weak evidence for solar Ne and Mg and twice solar Fe. Previous studies (Saizar et al. 1991 and Andreã et al. 1991, 1994) of PW Vul have yielded considerable differences in their derived elemental abundances for the ejecta. Our abundances fall in between the previous studies. To explain the discrepant abundances, we analyze in detail the data and methods used to obtain the previous results. The abundances of Saizar et al. (1991) are significantly smaller then our values because of the lower electron temperature used by Saizar et al. in deriving elemental abundances from ion abundances. Andreã et al. (1991) used an ionization correction method to obtain their abundances and ...

  4. Overview of the SuperNova/Acceleration probe (SNAP)

    Energy Technology Data Exchange (ETDEWEB)

    galdering@lbl.gov

    2002-07-29

    The SuperNova/Acceleration Probe (SNAP) is a space-based experiment to measure the expansion history of the Universe and study both its dark energy and the dark matter. The experiment is motivated by the startling discovery that the expansion of the Universe is accelerating. A 0.7 square-degree imager comprised of 36 large format fully-depleted n-type CCD's sharing a focal plane with 36 HgCdTe detectors forms the heart of SNAP, allowing discovery and lightcurve measurements simultaneously for many supernovae. The imager and a high-efficiency low-resolution integral field spectrograph are coupled to a 2-m three mirror anastigmat wide-field telescope, which will be placed in a high-earth orbit. The SNAP mission can obtain high-signal-to-noise calibrated light-curves and spectra for over 2000 Type Ia supernovae at redshifts between z = 0.1 and 1.7. The resulting data set can not only determine the amount of dark energy with high precision, but test the nature of the dark energy by examining its equation of state. In particular, dark energy due to a cosmological constant can be differentiated from alternatives such as ''quintessence'', by measuring the dark energy's equation of state to an accuracy of {+-} 0.05, and by studying its time dependence.

  5. A nova empresa e a informação

    Directory of Open Access Journals (Sweden)

    César Augusto Tibúrcio Silva

    2001-01-01

    Full Text Available Segundo Ronald Coase, as transações econômicas envolvem custos denominados de custos de transação. A melhor forma de a sociedade organizar-se é quando os custos de transação são os menores possíveis. As transações econômicas dentro da empresa são uma alternativa ao mercado ao reduzir esses custos. A explicação de Coase ajuda também a entender como a economia de escala pode favorecer o surgimento das grandes empresas modernas. As mudanças tecnológicas modernas alteraram, de forma substancial, o custo detransação. Isso faz com seja possível prognosticar o surgimento de uma nova empresa, mais focada no seu negócio típico. Diante disso, ao estudar a informação como um produto econômico pode-se fazer algumas inferências sobre como o custo da informação deve ser tratado tecnicamente. Finalmente são levantadas algumas conclusões.

  6. Surface Current Measurements In Terra Nova Bay By Hf Radar

    Science.gov (United States)

    Flocco, D.; Falco, P.; Wadhams, P.; Spezie, G.

    We present the preliminary results of a field experiment carried out within frame- work of the CLIMA project of the Italian National Programme for Antarctic Research (PNRA) and in cooperation with the Scott Polar Research Institute of Cambridge. Dur- ing the second period (02/12/1999-23/01/2000) of the XV Italian expedition a coastal radar was used to characterize the current field in the area of Terra Nova Bay (TNB). One of the aims of the CLIMA (Climatic Long-term Interactions for the Mass balance in Antarctica) project is to determine the role of the polynya in the sea ice mass bal- ance, water structure and local climate. The OSCR-II experiment was planned in order to provide surface current measurements in the area of TNB polynya, one of the most important coastal polynya of the Ross Sea. OSCR (Ocean Surface Current Radar) is a shore based, remote sensing system designed to measure sea surface currents in coastal waters. Two radar sites (a master and a slave) provide with radial current mea- surements; data combined from both sites yield the total current vector. Unfortunately the master and slave stations did not work together throughout the whole period of the experiment. A description of the experiment and a discussion of the results, will be proposed.

  7. Cyclic Period Oscillation of the Eclipsing Dwarf Nova DV UMa

    Science.gov (United States)

    Han, Z.-T.; Qian, S.-B.; Irina, Voloshina; Zhu, L.-Y.

    2017-05-01

    DV UMa is an eclipsing dwarf nova with an orbital period of ˜2.06 hr, which lies just at the bottom edge of the period gap. To detect its orbital period changes, we present 12 new mid-eclipse times by using our CCD photometric data and archival data. The latest version of the O-C diagram, combined with the published mid-eclipse times in quiescence, and spanning ˜30 years, was obtained and analyzed. The best fit to those available eclipse timings shows that the orbital period of DV UMa is undergoing a cyclic oscillation with a period of 17.58(+/- 0.52) years and an amplitude of 71.1(+/- 6.7) s. The periodic variation most likely arises from the light-travel-time effect via the presence of a circumbinary object, because the required energy to drive the Applegate mechanism is too high in this system. The mass of the unseen companion was derived as {M}3\\sin i\\prime =0.025(+/- 0.004) {M}⊙ . If the third body is in the orbital plane (i.e., i\\prime =i=82\\buildrel{\\circ}\\over{.} 9) of the eclipsing pair, this would indicate it is a brown dwarf. This hypothetical brown dwarf is orbiting its host star at a separation of ˜8.6 au in an eccentric orbit (e = 0.44).

  8. Superhumps in Cataclysmic Binaries. XXIV. Twenty More Dwarf Novae

    CERN Document Server

    Patterson, J; Kemp, J; Skillman, D R; Vanmunster, T; Harvey, D; Fried, R E; Jensen, L; Cook, L; Rea, R; Monard, B; McCormick, J; Velthuis, F; Walker, S; Martin, B; Bolt, G; Pavlenko, E P; O'Donoghue, D; Gunn, J; Novak, R; Masi, G; Garradd, G; Butterworth, N D; Krajci, T; Foote, J; Beshore, E

    2003-01-01

    We report precise measures of the orbital and superhump period in twenty more dwarf novae. For ten stars, we report new and confirmed spectroscopic periods - signifying the orbital period P_o - as well as the superhump period P_sh. These are GX Cas, HO Del, HS Vir, BC UMa, RZ Leo, KV Dra, KS UMa, TU Crt, QW Ser, and RZ Sge. For the remaining ten, we report a medley of P_o and P_sh measurements from photometry; most are new, with some confirmations of previous values. These are KV And, LL And, WX Cet, MM Hya, AO Oct, V2051 Oph, NY Ser, KK Tel, HV Vir, and RX J1155.4-5641. Periods, as usual, can be measured to high accuracy, and these are of special interest since they carry dynamical information about the binary. We still have not quite learned how to read the music, but a few things are clear. The fractional superhump excess epsilon [=(P_sh-P_o)/P_o] varies smoothly with P_o. The scatter of the points about that smooth curve is quite low, and can be used to limit the intrinsic scatter in M_1, the white dwarf ...

  9. RR Pictoris: an old nova showing superhumps and QPOs

    CERN Document Server

    Schmidtobreick, L; Tappert, C; Ederoclite, A

    2008-01-01

    We present time-resolved V-photometry of the old nova RR Pic. Apart from the hump-like variability, the light curves show the strong flickering and random variation typical for RR Pic. We do not find any convincing evidence for the previously reported eclipse. The extrapolated eclipse phase coincides with a broad minimum, but comparing the overall shape of the light curve suggests that the eclipse should actually be located around phase 0.2. The orbital period which we derive from these data agrees well with the old one, any uncertainty is too small to account for the possible phase shift. Apart from the 3.48h period, which is usually interpreted as the orbital one, we find an additional period at P=3.78h, which we interpret as the superhump period of the system; the corresponding precession period at 1.79d is also present in the data. We also find indications for the presence of a 13min quasi-periodic oscillation.

  10. Nova-like cataclysmic variables in the infrared

    Energy Technology Data Exchange (ETDEWEB)

    Hoard, D. W. [Eureka Scientific, Inc., Oakland, CA (United States); Long, Knox S. [Space Telescope Science Institute, Baltimore, MD (United States); Howell, Steve B. [NASA Ames Research Center, Moffett Field, CA (United States); Wachter, Stefanie [Max Planck Institut für Astronomie, D-69117 Heidelberg (Germany); Brinkworth, Carolyn S. [Spitzer Science Center, California Institute of Technology, Pasadena, CA (United States); Knigge, Christian [Physics and Astronomy, University of Southampton, Southampton (United Kingdom); Drew, J. E. [Centre for Astrophysics Research, Science and Technology Research Institute, University of Hertfordshire, Hatfield (United Kingdom); Szkody, Paula [Department of Astronomy, University of Washington, Seattle, WA (United States); Kafka, S. [Carnegie Institution of Washington, Department of Terrestrial Magnetism, Washington, DC (United States); Belle, Kunegunda [Los Alamos National Laboratory, Los Alamos, NM (United States); Ciardi, David R. [NASA Exoplanet Science Institute, California Institute of Technology, Pasadena, CA (United States); Froning, Cynthia S. [Center for Astrophysics and Space Astronomy, Department of Astrophysical and Planetary Sciences, University of Colorado, Boulder, CO (United States); Van Belle, Gerard T. [Lowell Observatory, Flagstaff, AZ (United States); Pretorius, M. L., E-mail: hoard@mpia.de [Department of Physics, University of Oxford, Oxford (United Kingdom)

    2014-05-01

    Nova-like (NL) cataclysmic variables have persistently high mass transfer rates and prominent steady state accretion disks. We present an analysis of infrared observations of 12 NLs obtained from the Two Micron All Sky Survey, the Spitzer Space Telescope, and the Wide-field Infrared Survey Explorer All Sky Survey. The presence of an infrared excess at λ ≳ 3-5 μm over the expectation of a theoretical steady state accretion disk is ubiquitous in our sample. The strength of the infrared excess is not correlated with orbital period, but shows a statistically significant correlation (but shallow trend) with system inclination that might be partially (but not completely) linked to the increasing view of the cooler outer accretion disk and disk rim at higher inclinations. We discuss the possible origin of the infrared excess in terms of emission from bremsstrahlung or circumbinary dust, with either mechanism facilitated by the mass outflows (e.g., disk wind/corona, accretion stream overflow, and so on) present in NLs. Our comparison of the relative advantages and disadvantages of either mechanism for explaining the observations suggests that the situation is rather ambiguous, largely circumstantial, and in need of stricter observational constraints.

  11. An Emerging Wine Region in Nova Scotia, Canada: Terroir Trials and Tribulations

    Science.gov (United States)

    Cameron, B. I.; Ketter, B. S.; Karakis, S.

    2012-12-01

    Nova Scotia, strategically located on Canada's east coast, is an emerging wine region, whose distinctive wines are garnering international acclaim. Nova Scotia has a long and rich tradition of growing grapes for wine dating back as far as 1611. Nova Scotia's mesoclimates, glacial soils, and proximity to the Atlantic Ocean form a complex alliance to create a unique and expressive terroir. Tidal Bay is a new appellation wine for Nova Scotia stylistically defined as a fresh, crisp and high-acid blend of white grapes. There are four main wine-growing regions in Nova Scotia, all influenced by the warming effects of the Bay of Fundy and Atlantic Ocean: Malagash Peninsula, Annapolis Valley, Bear River Valley and the South Shore. Nova Scotia currently has 14 producing wineries with many more in the development stage. Nova Scotia grape growers not only have had success developing mature and consistent hybrids, but in recent years several vinifera have flourished in this cool climate area. The white hybrids include L'Acadie Blanc, New York Muscat, Seyval Blanc, and Vidal Blanc. The white vinifera include chardonnay, riesling, pinot gris, and sauvignon blanc. Red hybrids are Baco Noir, Leon Millet, Lucie Kuhlmann, and Marechal Foch, whereas the only red vinifera is pinot noir. Nova Scotia has nearly perfect climatic conditions for making world class icewines and sparkling wines. A preliminary GIS analysis of climate, topographic, geology and soil data helps to define Nova Scotia's terroir. Annual precipiatation varies from 10 to 21.6 cm/year with a vast majority of the wineries located in regions with the lowest rainfall. Daily average temperature ranges from 5.5 to 7.5°C, degree growing days above 5°C from 1382 to 1991, and mean August temperature from 15.6 to 19.3 °C. Wineries cluster in the warmest regions based on these temperature measures to assist grape ripening. Soils in these diverse wine regions can range from silty, sandy and clay loams to more gravel-rich sandy

  12. Características das fibras musculares de cordeiros nascidos de ovelhas recebendo suplementação proteica no terço inicial da gestação Characteristics of muscle fibers of lambs born from sheep given protein suplementation in the intial third of pregnancy

    OpenAIRE

    2010-01-01

    Foram utilizadas 80 ovelhas Santa Inês, com 47,49 ± 3,76 kg de peso vivo, cobertas com reprodutores Dorper e alimentadas com concentrado com 15,20; 22,48; 26,52 e 35,65% de proteína bruta (PB) no terço inicial de gestação. As ovelhas, durante o dia, permaneceram em pastagem de capim-aruana (Panicum maximum cv. Aruana). Ao nascimento, foram realizadas biópsias no músculo Semitendinosus esquerdo de cordeiros machos, para avaliar o número e o diâmetro das fibras musculares. Na fase de terminação...

  13. Rendimentos de carcaça, composição tecidual e musculosidade da perna de cordeiros alimentados com silagem de milho ou cana-de-açúcar em dois níveis de concentrado Carcass yield, tissue composition, and leg muscularity of lambs fed corn silage or sugar cane in two levels of concentrate

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    G.M.B. Moreno

    2010-06-01

    Full Text Available Avaliou-se o efeito da relação volumoso:concentrado e do tipo de volumoso nos rendimentos de carcaça e dos cortes comerciais, e sobre a composição dos tecidos e musculosidade da perna de 32 cordeiros Ile de France, terminados em confinamento, alimentados com silagem de milho ou cana-de-açúcar, em duas relações volumoso:concentrado: de 60:40 ou 40:60. Os cordeiros foram abatidos aos 32kg de peso corporal; calcularam-se o peso e o rendimento da carcaça quente (PCQ e RCQ. Após 24 horas de refrigeração, obtiveram-se o peso e o rendimento da carcaça fria (PCF e RCF, o rendimento verdadeiro e as perdas por resfriamento. As carcaças foram divididas em cinco cortes comerciais, paleta, lombo, perna, costelas e pescoço, e a perna foi dissecada em músculo, osso e gordura, calculando-se as relações músculo:osso e músculo:gordura, além do índice de musculosidade da perna. Os cordeiros alimentados com silagem de milho apresentaram maiores PCQ (16,05kg, PCF (15,61kg, RCQ (50,4% e RCF (49,0%. O rendimento de lombo foi menor nos cordeiros alimentados com cana-de-açúcar (9,1%. A cana-de-açúcar e a silagem de milho nas duas relações volumoso:concentrado estudadas não afetaram as proporções de osso, músculo e gordura e musculosidade da perna, e podem constituir a dieta desses animais sem diminuir as proporções desses tecidos, responsáveis pela qualidade da carne.The effects of roughage:concentrate ratio and type of roughage were evaluated on the carcass yield and commercial cuts, and tissue composition and leg muscularity of 32 Ile de France lambs finished in feedlot and fed corn silage or sugar cane in two roughage:concentrate ratios: 60:40 or 40:60. The lambs were slaughtered with 32kg of body weight and the weight and yield of hot carcass (WHC and YHC were determined. After refrigerated for 24h in cold camera, the weight and yield of cold carcass (WCC and YCC, real yield, and weight loss for cooling were obtained. The carcass

  14. Composição corporal e exigências líquidas em energia e proteína para ganho de cordeiros de quatro grupos genéticos Body composition and net protein and energy requirements of four genetic groups of lambs

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    André Nunes de Oliveira

    2004-10-01

    Full Text Available O estudo foi conduzido no Setor de Ovinocultura do Departamento de Zootecnia da Universidade Federal de Lavras, Minas Gerais, onde foi avaliada a composição corporal em proteína, gordura e energia e estimadas as exigências líquidas de proteína e energia para ganho de peso de cordeiros. Foram utilizados 48 cordeiros machos, não castrados, Santa Inês puros (SI e cruzados Texel x Santa Inês (TxSI, Ile de France x Santa Inês (IFxSI e Bergamácia x Santa Inês (BxSI, mantidos em confinamento e abatidos aos 15, 25, 35 e 45 kg de peso vivo (PV. Foram ajustadas equações da quantidade corporal de proteína, gordura e energia, em função do logaritmo do peso corporal vazio (PCVZ. As exigências líquidas em proteína e energia para ganho de peso foram obtidas por derivação das equações de predição da composição corporal em proteína e energia. Foi realizado um teste de comparação dos coeficientes de regressão das equações logarítmicas obtidas, o qual detectou diferenças entre os cordeiros TxSI e os demais. Para todos os grupos genéticos avaliados, o conteúdo corporal de proteína diminuiu, ao passo que os conteúdos de gordura e energia aumentaram à medida que o PCVZ elevou-se. Os cordeiros TxSI apresentaram maiores exigências protéicas e energéticas para ganho de peso do que os SI, IFxSI e BxSI.This study was carried out at the Sheep Sector of the Animal Production Department of the Federal University of Lavras, Minas Gerais. The protein, fat and energy body content was evaluated and the net requirements of protein and energy for weight gain of lambs were determined. Forty-eight uncastrated male lambs, pure Santa Inês (SI and crossed Texel x Santa Inês (TxSI, Ile de France x Santa Inês (IFxSI and Bergamácia x Santa Inês (BxSI, maintained in feedlot and slaughtered to the 15, 25, 35 and 45 kg of live weight, were used. Regression analyses of the logarithm of protein, fat and energy body content in function of the

  15. Consumo de nutrientes e desempenho de cordeiros alimentados com dietas que contêm diferentes níveis de fibra em detergente neutro Intake of nutrients and performance of lambs fed with diets containing different levels of neutral detergent fiber

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    Adriano Ramos Cardoso

    2006-02-01

    Full Text Available Este estudo foi conduzido no Departamento de Zootecnia da Universidade Federal de Santa Maria, RS, no período de agosto a dezembro de 2003. O objetivo foi avaliar o consumo de nutrientes e o desempenho de cordeiros machos, não castrados, cruzados Ile de France x Texel, submetidos a quatro níveis de fibra em detergente neutro (FDN: 25%, 31%, 37% e 43%. O volumoso utilizado foi a silagem de sorgo híbrido (AG 2005 E e o concentrado foi composto de milho em grão triturado, farelo de soja, sal comum, calcário calcítico e fosfato bicálcico. As dietas dos quatro tratamentos eram isoprotéicas, contendo 17% de proteína bruta. Foram utilizados 20 cordeiros desmamados em média aos 42 dias de idade e abatidos quando atingiram 30kg de peso vivo. O delineamento experimental foi o inteiramento casualizado, com quatro tratamentos e cinco repetições. Foram avaliados os consumos de nutrientes, o ganho de peso médio diário (GMD, a conversão alimentar (CA e o número de dias que os cordeiros levaram para atingir o peso vivo ao abate de 30kg. A adição de níveis crescentes de FDN à dieta ocasionou um decréscimo linear nos consumos de matéria seca, matéria orgânica, proteína bruta, extrato etéreo, carboidratos totais e carboidratos não estruturais. Por outro lado, aumentou linearmente o consumo de fibra em detergente neutro e fibra em detergente ácido. Verificou-se redução linear do GMD e piora na CA com o aumento do teor de fibra na ração, o que proporcionou uma elevação linear no número de dias que os cordeiros levaram para atingir o peso de abate.This study was conducted at the Animal Science Department of Federal University of Santa Maria, RS, from August to December 2003. The aim was to evaluate the food intake and performance of male lambs, non-castrated, crossbreed Ile de France x Texel, submitted to four levels of NDF: 25%, 31%, 37% and 43%. The roughage used was a hybrid sorghum silage (AG 2005 E and the concentrate was

  16. Produção de cordeiros em pastagem de azevém e trevo-branco sob diferentes níveis de resíduos de forragem Lamb production in a mixture of italian ryegrass and white clover under different forage mass levels

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    Marcos Weber do Canto

    1999-02-01

    Full Text Available Na presente pesquisa, objetivou-se analisar os efeitos de diferentes níveis de resíduos de forragem na produção de cordeiros. O experimento foi estabelecido em Tupanciretã, região do Planalto Médio do Estado do Rio Grande do Sul, em uma pastagem de azevém cv. Estanzuela 284 (Lolium multiflorum Lam + trevo-branco cv. Yi (Trifolium repens L., submetida a diferentes níveis de resíduo de matéria seca (RMS. O delineamento experimental utilizado foi o completamente casualizado, estudando-se os níveis de RMS mantidos na pastagem de 1.119, 1.320, 1.477, 1.695, 2.146, 2.166, 2.410 e 2.483 kg de matéria seca por hectare (MS/ha. O período experimental foi de 30/09 a 08/12/1992 e os animais utilizados foram cordeiros cruza Ile de France x Corriedale desmamados aos 80 dias. Foram avaliados o ganho de peso médio diário (GMD, ganho de peso vivo/ha (GPV/ha, carga animal, animais dia/ha e a eficiência de conversão de MS em kg de peso vivo de cordeiros. Os resultados obtidos mostraram uma relação linear positiva entre o GMD e GPV/ha com o aumento nos níveis de RMS/ha, observando-se nos níveis de RMS superiores a 2.400 kg um GMD de 0,12 kg/cordeiro/dia e um GPV/ha médio de 497 kg. Não houve relação quanto à carga animal e animais.dia/ha; verificou-se uma relação linear negativa entre a eficiência de conversão de MS com os níveis de RMS estudados. Os resultados demonstram o efeito dos níveis de RMS na resposta animal.The objective of this research was to analyse the effects of different forage mass levels on lamb production. The experiment was conducted in Tupanciretã, Planalto Médio region at the State of Rio Grande do Sul, Brazil, in a mixture of italian ryegrass cv. Estanzuela 284 (Lolium multiflorum Lam. + white clover cv. Yi (Trifolium repens L., under different forage mass (FM levels. The experimental design used was completely randommized, and the FM levels studied were: 1,119, 1,320, 1,477, 1,695, 2,146, 2,166, 2,410 and 2

  17. Avaliação das proporções dos cortes da carcaça, características da carne e avaliação dos componentes do peso vivo de cordeiros Evaluation of carcass cuttings proportion, meat characteristics and evaluation of live weight components of lambs

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    Rafael Batista Medeiros Frescura

    2005-02-01

    Full Text Available Objetivou-se, neste trabalho, avaliar a composição física da carcaça, as características da carne e a proporção dos não-componentes da carcaça do peso vivo de cordeiros abatidos aos 28 kg submetidos a diferentes sistemas alimentares. Dezoito cordeiros (Ile de France x Texel foram distribuídos aleatoriamente, com as respectivas mães, em três tratamentos: PCA - pastagem cultivada de azevém (Lolium multiflorum Lam., CON - confinamento sem alimentação privativa e CCF - confinamento com alimentação privativa para os cordeiros. A alimentação privativa foi oferecida aos cordeiros pelo sistema de creep feeding. Não houve diferença para o percentual do pescoço entre PCA, CON e CCF, com valores de 9,27; 9,17 e 8,72%, respectivamente. Para o percentual de perna, os animais da CON (34,02% e CCF (34,17% apresentaram valores semelhantes entre si e superiores aos da PCA (31,73%. A maciez medida na porção do Longissimus dorsi entre a 9ª e 12ª costelas foi semelhante entre os animais dos três tratamentos, de 2,33; 3,03 e 3,08 para PCA, CON e CCF, respectivamente. Não houve efeito dos tratamentos sobre a palatabilidade e suculência da carne. O percentual de pele dos animais da PCA (11,05% e do CON (10,50% foram semelhantes entre si, enquanto o PCA apresentou valores mais elevados que o percentual dos animais do CCF (9,70%. Para o percentual do conteúdo gástrico, os valores observados para os animais do CCF (11,47% foram superiores àqueles da PCA (5,09% e semelhantes aos obtidos para os animais do CON (8,72%.This study aimed to evaluate carcass physical comp0sition, meat characteristics and live weight carcass no component of lambs slaughter at 28 kg under different feeding systems. Eighteen lambs (Ile de France X Texel were randomly allotted, with their respective mothers, to three treatments: RP - ryegrass pasture (Lolium multiflorum Lam., COM - confinament of lamb and sheep together and CCF - confinament with creep feeding. A

  18. Comportamento ingestivo de cordeiros e digestibilidade dos nutrientes de dietas contendo alta proporção de concentrado e diferentes fontes de fibra em detergente neutro Lamb feeding behavior and nutrient digestibility of high concentrate diets with different neutral detergent fiber sources

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    Clayton Quirino Mendes

    2010-03-01

    Full Text Available Dois experimentos foram realizados para avaliar os efeitos da substituição da fibra em detergente neutro (FDN do bagaço de cana-de-açúcar in natura pela FDN da casca de soja em dietas com alta proporção de concentrado sobre o comportamento ingestivo de cordeiros e a digestibilidade dos nutrientes. No primeiro experimento, 60 cordeiros com 16,4 ± 0,3 kg de peso corporal e idade inicial de 67 ± 2 dias foram distribuídos em delineamento de blocos completos casualizados, em esquema fatorial 2 × 2 + 1, composto de duas fontes de FDN (bagaço de cana in natura ou casca de soja, dois teores de FDN (14 ou 18% e uma dieta controle contendo 100% de concentrado. No segundo experimento, cinco cordeiros foram distribuídos em quadrado latino 5 × 5 e submetidos às mesmas dietas do experimento 1. As dietas contendo as fontes de fibra promoveram maior consumo de matéria seca, matéria orgânica e FDN e maior tempo de ingestão, ruminação e mastigação (minutos/dia em comparação à dieta contendo 100% de concentrado. As dietas contendo o bagaço de canade-açúcar in natura proporcionaram maior atividade de ruminação que aquelas com casca de soja. Entretanto, a utilização da casca de soja proporcionou menor atividade de mastigação e maior digestibilidade dos nutrientes em relação ao bagaço de cana-de-açúcar in natura. A casca de soja pode ser utilizada como única fonte adicional de FDN em dietas contendo alto teor de concentrado para cordeiros.Two experiments were performed to determine the effects of replacing the neutral detergent fiber from sugarcane bagasse with soybean hulls neutral detergent fiber in high concentrate diets on lamb feeding behavior and apparent nutrient digestibility. In the first experiment, 60 ram lambs with 16.4 ± 0.3 kg body weight and 67 ± 2 days old were allotted to a complete randomized block design as a 2 × 2 + 1 factorial arrangement of treatments, consisting of two neutral detergent fiber sources

  19. Desempenho de cordeiros das raças Bergamácia e Santa Inês, terminados em confinamento, recebendo dejetos de suínos como parte da dieta Performance of Bergamácia and Santa Inês lambs, finished in fedlot, receiving swine wastes as part of diet

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    Marcus Vinícius Morais de Oliveira

    2003-12-01

    Full Text Available Foram confinados, individualmente 33 cordeiros das raças Bergamácia e Santa Inês, por um período de 75 dias, com o intuito de avaliar a influência da raça e a viabilidade de utilizar dejetos de suínos como parte da dieta, sobre o consumo e desempenho de cordeiros terminados em confinamento. Utilizaram-se dois tipos de dejetos: o Bijú (Dejeto obtido através da raspagem e varredura do piso das baias de crescimento e terminação e o Dejeto Peneirado Seco - DPS (Dejeto obtido através da peneiração da parte sólida do material contido na lâmina d'água e na água da lavagem das baias. Os tratamentos foram: T1- Controle; T2- Dieta com 24 % de Bijú; e T3- Dieta com 24 % de DPS. O ganho de peso (GP e conversão alimentar (CA foram afetados negativamente com o uso de dejetos de suínos, todavia o consumo proteína bruta (PB e cálcio (Ca não foi influenciado. Houve maior consumo de fósforo (P nas dietas contendo dejetos, sendo o consumo de fibra em detergente neutro (FDN e extrato etéreo (EE variável. Entre as rações que continham dejetos não foram verificadas diferenças sobre os consumos de MS, PB, Ca e P e sobre o GP. Os cordeiros da raça Bergamácia apresentaram maior GP que os cordeiros da raça Santa Inês.Thirty three lambs of Bergamácia and Santa Inês the breeds were individually confined for a period of 75 days with the objective to evaluate the influence of breed and the viability of the use of swine wastes as part of the diet on the intake and performance of lambs. Two types of wastes were used: Bijú (Wastes obtained through the scratching and sweeping of the floor of the growth and termination stalls and the Dry Sifted Wastes - DSW (Wastes obtained through the sifting of the solid part of the material contained in the of water sheet of the stalls and in the water of washing of the stalls. The treatments were: T1- Control; T2- Diet with 24% of Bijú; and T3- Diet with 24% of DSW, dry matter base. There was influence

  20. Desempenho, características de carcaça e resultado econômico de cordeiros criados em creep feeding com silagem de grãos úmidos de milho Live weight gain, carcass traits and economic results on lambs fed with high moisture corn silage in creep feeding

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    Gercílio Alves de Almeida Júnior

    2004-08-01

    Full Text Available Objetivou-se, com este trabalho, estudar níveis de substituição (0; 50 e 100% do milho grão seco moído pela silagem de grãos úmidos de milho na ração de cordeiros alimentados em creep feeding. Vinte e quatro cordeiros Suffolk foram avaliados quanto ao desempenho, pesos e rendimentos das carcaças. Também foi realizada uma análise econômica. As rações foram fornecidas ad libitum, sendo suas sobras pesadas para o cálculo do consumo médio por animal. Ao atingirem 28 kg de peso vivo, os cordeiros foram submetidos a jejum por 16 horas e, então, novamente pesados para se obter o peso vivo ao abate. Após o abate, os animais foram eviscerados para se obterem os pesos e rendimentos de carcaça quente. As carcaças permaneceram por 24 horas em câmara de refrigeração, sendo novamente pesadas para se obterem os rendimentos de carcaça fria e as perdas por resfriamento. Os resultados revelaram que não houve efeito dos níveis de substituição sobre ganho médio diário de peso vivo, idade ao abate, pesos e rendimentos das carcaças quentes e frias, indicando que a silagem de grãos úmidos de milho pode ser utilizada em substituição ao milho moído na alimentação de cordeiros. Como o peso ao abate foi pré-fixado, as variações nas idades ao abate fizeram com que essa variável exercesse influência sobre os desempenhos, pesos e rendimentos e, quanto maiores essas idades, piores os resultados dos parâmetros avaliados. O tratamento com 50% de silagem de grãos úmidos apresentou os melhores resultados econômicos e o tratamento sem silagem de grãos úmidos foi o de menor rentabilidade.The experiment was carried to study three levels (0, 50 e 100% of high moisture corn silage replacing dry corn grain in rations of lambs fed in creep feeding. Twenty four Suffolk lambs were evaluated to live weight (LW gain and carcasses dressing-outs percentage. It was performed an economical analysis too. Rations in creep feeding were fed ad

  1. Composição tecidual e centesimal e teor de colesterol da carne de cordeiros terminados em confinamento com dietas contendo níveis crescentes de resíduo úmido de cervejaria Tissue and centesimal composition and cholesterol of the meat of lambs feedlot with diets with different levels of brewery's residue

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    Sérgio Carvalho

    2008-10-01

    Full Text Available Este estudo teve como objetivo avaliar a influência de diferentes níveis de substituição do alimento concentrado por resíduo úmido de cervejaria sobre a composição tecidual, a composição centesimal e o teor de colesterol da carne de cordeiros terminados em confinamento. Foram utilizados 25 cordeiros, machos, não-castrados, da raça Texel, distribuídos aleatoriamente em cinco tratamentos compostos por níveis de substituição do alimento concentrado por resíduo úmido de cervejaria, sendo: 0%, 25%, 50%, 75% e 100% de substituição. Foram utilizadas uma dieta composta de feno de Tifton-85 e uma mistura concentrada em uma relação volumoso: concentrado de 40:60, com base na matéria seca (MS. O alimento concentrado foi constituído por milho desintegrado, farelo de soja, mistura mineral e resíduo úmido de cervejaria, sendo que suas proporções variaram de acordo com os tratamentos. As dietas foram formuladas para serem isoprotéicas, baseados no teor de proteína bruta (PB do tratamento com maior nível de resíduo. Os cordeiros foram abatidos após um período experimental de 77 dias. Observou-se, na secção entre a 9ª e a 11ª costelas, que os pesos de osso, músculo e gordura diminuíram linearmente e a proporção de músculo aumentou linearmente com o incremento do nível de resíduo. Verificou-se aumento linear na proporção de umidade no músculo Longissimus dorsi com o aumento do resíduo úmido de cervejaria nas dietas dos cordeiros.The purpose of this experiment was to evaluate the influence of different levels of substitution of the concentrate by brewery's residue on the tissue composition, centesimal composition and cholesterol content in the meat of lambs finished in feedlot. Twenty-five male, non castrated Texel lambs were used, distributed in five treatments, which consisted in the levels of brewery's residue replacing concentrate, being 0%, 25%, 50%, 75% and 100% of substitution. Diet's composition was Tifton

  2. Desempenho de cordeiros Santa Inês alimentados com dietas completas contendo feno de maniçoba Performance of Santa Inês lambs fed total mixed rations containing different ratios of concentrate to ceara rubbertree hay

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    Jacilene Maria da Cunha Castro

    2007-06-01

    Full Text Available Avaliou-se o desempenho de cordeiros alimentados com dieta completa formulada com diferentes proporções de feno de maniçoba. Foram utilizados 32 animais Santa Inês machos, não-castrados (idade inicial de 70 dias e peso vivo de 16,02±2,37 kg, distribuídos em delineamento inteiramente casualizado, com quatro tratamentos e oito repetições. As dietas foram constituídas de concentrado e feno de maniçoba (FM nas proporções de 20, 40, 60 e 80%. As proporções de feno na dieta não influenciaram os consumos de MS, PB e CT, cujas médias diárias foram 1,214; 0,201 e 0,816 kg, respectivamente. Os níveis de feno tiveram efeito linear positivo sobre o consumo de FDN e efeito linear negativo sobre o consumo de EM e CNF. O ganho de peso diário foi afetado pelos níveis de feno na dieta, apresentando médias de 290,84; 293,62; 253,35 e 208,48 g, respectivamente, para as dietas com 20, 40, 60 e 80% de feno de maniçoba. As dietas influenciaram a conversão (Y = 3,332+0,028x e a eficiência alimentar (Y = 0,280,0013x. Pela análise econômica, observaram-se relações custo:benefício de 1,49; 1,57; 1,69 e 1,84 para os níveis de 20, 40, 60 e 80% de feno de maniçoba na dieta. O custo operacional efetivo por quilograma de carcaça produzida foi de R$ 3,68; R$ 3,49; R$ 3,23 e R$ 2,98, respectivamente, para as dietas com 20, 40, 60 e 80% de feno. A inclusão de 80% de feno de maniçoba em dietas completas possibilitou a obtenção de desempenho satisfatório dos cordeiros e melhor retorno financeiro.The objective of this trial was to investigate the effect of different dietary ratios of concentrate (C to ceara rubbertree hay (CRH; Manihot Glaziovii Muell. Arg. on performance of lambs. Thirty two intact Santa Inês lambs averaging 70 days of age and 16.02±2.371 kg of body weight were fed one of the following four treatments as total mixed rations: 80C:20CRH (diet A, 60C:40CRH (diet B, 40C:60CRH (diet C, or 20C:80CRH (diet D in a completely

  3. Isotopic 32S/33S ratio as a diagnostic of presolar grains from novae

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    A. Parikh

    2014-10-01

    Full Text Available Measurements of sulphur isotopes in presolar grains can help to identify the astrophysical sites in which these grains were formed. A more precise thermonuclear rate of the 33S(p,γ34Cl reaction is required, however, to assess the diagnostic ability of sulphur isotopic ratios. We have studied the 33S(3He,d34Cl proton-transfer reaction at 25 MeV using a high-resolution quadrupole–dipole–dipole–dipole magnetic spectrograph. Deuteron spectra were measured at ten scattering angles between 10° and 55°. Twenty-four levels in 34Cl over Ex=4.6–5.9 MeV were observed, including three levels for the first time. Proton spectroscopic factors were extracted for the first time for levels above the 33S + p threshold, spanning the energy range required for calculations of the thermonuclear 33S(p,γ34Cl rate in classical nova explosions. We have determined a new 33S(p,γ34Cl rate using a Monte Carlo method and have performed new hydrodynamic nova simulations to determine the impact on nova nucleosynthesis of remaining nuclear physics uncertainties in the reaction rate. We find that these uncertainties lead to a factor of ≤5 variation in the 33S(p,γ34Cl rate over typical nova peak temperatures, and variation in the ejected nova yields of SCa isotopes by ≤20%. In particular, the predicted 32S/33S ratio is 110–130 for the nova model considered, compared to 110–440 with previous rate uncertainties. As recent type II supernova models predict ratios of 130–200, the 32S/33S ratio may be used to distinguish between grains of nova and supernova origin.

  4. The rms-flux relation in accreting white dwarfs: another nova-like variable and the first dwarf nova

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    Van de Sande, M; Knigge, C

    2015-01-01

    We report on the detection of the linear rms-flux relation in two accreting white dwarf binary systems: V1504 Cyg and KIC 8751494. The rms-flux relation relates the absolute root-mean-square (rms) variability of the light curve to its mean flux. The light curves analysed were obtained with the Kepler satellite at a 58.8 s cadence. The rms-flux relation was previously detected in only one other cataclysmic variable, MV Lyr. This result reenforces the ubiquity of the linear rms-flux relation as a characteristic property of accretion-induced variability, since it has been observed in several black hole binaries, neutron star binaries and active galactic nuclei. Moreover, its detection in V1504 Cyg is the first time the rms-flux relation has been detected in a dwarf nova-type CV during quiescence. This result, together with previous studies, hence points towards a common physical origin of accretion-induced variability, independent of the size, mass, or type of the central accreting compact object.

  5. Crescimento alométrico de osso, músculo e gordura em cortes da carcaça de cordeiros Texel segundo os métodos de alimentação e peso de abate Muscle, fat and bone allometric growth in Texel lambs carcasses cuts in relation to the feeding methods and slaughter weight

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    Gilberto Teixeira da Rosa

    2005-08-01

    Full Text Available O experimento teve como objetivo estudar o crescimento alométrico dos diferentes tecidos do pescoço, costela, paleta e perna em relação ao peso do corte de cordeiros e cordeiras. Foram utilizados 22 machos inteiros e 23 fêmeas da raça Texel. Desses, sete foram abatidos no início do experimento e os demais, aos pesos de 25 ou 33kg. As ovelhas mais cordeiros foram distribuídos em três métodos de alimentação: M1 -Silagem de milho e concentrado, apenas aos cordeiros até o desmame, aos 60 dias; M2 - Silagem de milho e concentrado, apenas aos cordeiros até o desmame, aos 45 dias e M3 - Silagem de milho e concentrado para ovelha mais cordeiro até o desmame com 60 dias. Após o desmame, os cordeiros receberam silagem mais concentrado. Foi utilizado um delineamento inteiramente casualizado em arranjo fatorial 3 x 2 x 2 (3 métodos, 2 sexos e 2 pesos de abate. A determinação do crescimento foi obtida através da equação log y = log.a + b log.x, utilizando-se o logaritmo do peso de osso, músculo e gordura em função do logaritmo do peso do corte. Observou-se que o osso do pescoço e da costela foram precoce (b1 independente de sexo e método de alimentação com coeficientes de alometria variando de 1,78 a 2,15 (pescoço e 1,51 a 1,65 (costela. Na paleta, o osso foi precoce em ambos os sexos, com coeficientes de alometria variando de 0,76 a 0,79 e 0,54 a 0,58 respectivamente para machos e fêmeas. O músculo apresentou crescimento isométrico (b=1, independente de sexo e peso de abate. A gordura foi tardia (b>1 independente de peso de abate e sexo, com coeficientes de alometria variando de 1,80 a 2,12. Na perna o osso apresentou crescimento precoce nas fêmeas e isométricas nos machos, com coeficientes de alometria variando de 0,57 a 0,63 e 0,78 a 0,80 respectivamente para ambos os sexos O músculo apresentou crescimento isométrico (b=1, independente de sexo e peso de abate. A gordura foi tardia (b>1 independente de peso de abate e

  6. Desempenho e avaliação econômica da alimentação de cordeiros confinados com dietas contendo diferentes relações volumoso: concentrado Performance and economic evaluation of the feeding of feedlot lambs with diets with different roughage: concentrate ratios

    Directory of Open Access Journals (Sweden)

    Sérgio Carvalho

    2007-10-01

    Full Text Available Este estudo objetivou avaliar o efeito do uso de diferentes relações volumoso:concentrado sobre o desempenho, as características de carcaça e o conteúdo gastrintestinal de cordeiros, bem como realizar uma avaliação econômica da alimentação de cordeiros confinados na fase de terminação. Foram utilizados 25 cordeiros, machos não-castrados, da raça Texel, desmamados com a idade média de 60 dias, e distribuídos aleatoriamente em cinco tratamentos, compostos por diferentes relações volumoso:concentrado, sendo: 30:70; 40:60; 50:50; 60:40 e 70:30, em base da matéria seca (MS. O volumoso utilizado foi o feno de Tifton-85 e o alimento concentrado era constituído por ração comercial, farelo de soja, calcário calcítico e fosfato bicálcico, em diferentes proporções. O período experimental teve duração de 80 dias, quando os animais foram abatidos. O aumento do teor de volumoso e a diminuição no teor de concentrado nas dietas promoveu redução linear (P£0,01 no ganho de peso diário e peso vivo ao abate. O consumo de matéria seca e a conversão alimentar foram influenciados de forma quadrática pelo aumento da relação volumoso:concentrado. Verificou-se redução linear (P£0,01 no peso de carcaça quente, rendimento de carcaça quente e nos pesos de quarto (perna, paleta, costilhar, pescoço e de vísceras verdes vazias, com o aumento do teor de volumoso e a diminuição no teor de concentrado nas dietas. Ocorreu crescimento linear nas proporções de vísceras verdes cheias (P£0,05 e de conteúdo gastrintestinal (P£0,01 com a elevação da proporção de volumoso e com a redução na proporção de concentrado nas dietas. A lucratividade em relação à venda dos cordeiros vivos não diferiu entre os tratamentos, apresentando um valor médio de R$ 57,00 por cordeiro. Houve redução linear (P£0,05 na lucratividade em relação à venda das carcaças dos cordeiros com o aumento da proporção de volumoso e com a diminui

  7. Novas possibilidades discursivas na publicidade: diversidade em questao

    Directory of Open Access Journals (Sweden)

    Soares Bezerra, Josenildo

    2014-07-01

    Full Text Available A publicidade brasileira vem assumindo novos discursos que contemplam o consumidor em seu exercício da diversidade. Este artigo vislumbra discutir as mudanças estético-conceituais que a pós-modernidade nos apresenta. A publicidade vê nessas práticas discursivas, novas possibilidades de consumo, respeitando o sujeito em seu exercício subjetivo. Comerciais que contemplam experiências de novos conceitos de família, de gênero, etnia, bem como, os ditos para além da norma social, estão aparecendo como estilo de vida. Objetivamos trazer a discussão da publicidade enquanto lócus de visibilização das possibilidades experienciadas que subjetivam os sujeitos-consumidores sem apresentá-las em dissimetria com os consumidores adeptos aos discursos padronizados do eurocentrismo e heteronormativos. Esse trabalho tem como metodologia, os anúncios da empresa de cosmético Natura que traz VT’s em que o corpo revela suas possibilidades de estar no mundo, bem como comerciais da Renault e Pepsy demonstrando questões vinculadas às relações homoafetivas e étnico-raciais. Buscamos reflexões sócio-filosóficas ancoradas no discurso de linha francesa e foucaultiano, como também, leituras em Bauman acerca da modernidade líquida e Lipovetsky na perspectiva do hiperconsumo produtor da felicidade. Concluímos assim, apontando mudanças no consumo de bens e serviços, bem como, inserção de públicos ditos excluídos no cenário discursivo publicitário. Isto produz consumidores abertos ao respeito do diverso no campo publicitário e do consumo.

  8. Outburst-related period changes of recurrent nova CI aquilae

    Energy Technology Data Exchange (ETDEWEB)

    Wilson, R. E.; Honeycutt, R. K., E-mail: honey@astro.indiana.edu, E-mail: rewilson@ufl.edu [Astronomy Department, Indiana University, Swain Hall West, Bloomington, IN 47405 (United States)

    2014-11-01

    Pre-outburst and post-outburst light curves and post-outburst eclipse timings are analyzed to measure any period (P) change related to nova CI Aql's outburst of early 2000 and a mean post-outburst dP/dt, which then lead to estimates of the accreting component's rate of mass (M) change and its overall outburst-related change of mass over roughly a decade of observations. We apply a recently developed procedure for unified analysis of three timing-related data types (light curves, radial velocities, and eclipse timings), although with only light curves and timings in this case. Fits to the data are reasonably good without need for a disk in the light-curve model, although the disk certainly exists and has an important role in our post-outburst mass flow computations. Initial experiments showed that, although there seems to be an accretion hot spot, it has essentially no effect on derived outburst-related ΔP or on post-outburst dP/dt. Use of atomic time (HJED) in place of HJD also has essentially nil effect on ΔP and dP/dt. We find ΔP consistently negative in various types of solutions, although at best only marginally significant statistically in any one experiment. Pre-outburst HJD {sub 0} and P results are given, as are post-outburst HJD {sub 0}, P, and dP/dt, with light curves and eclipse times as joint input, and also with only eclipse time input. Post-outburst dP/dt is negative at about 2.4σ. Explicit formulae for mass transfer rates and epoch-to-epoch mass change are developed and applied. A known offset in the magnitude zero point for 1991-1994 is corrected.

  9. NASA Opportunities in Visualization, Art, and Science (NOVAS)

    Science.gov (United States)

    Fillingim, M. O.; Zevin, D.; Croft, S.; Thrall, L.; Shackelford, R. L., III

    2015-12-01

    Led by members of UC Berkeley's Multiverse education team at the Space Sciences Laboratory (http://multiverse.ssl.berkeley.edu/), in partnership with UC Berkeley Astronomy, NASA Opportunities in Visualization, Art and Science (NOVAS) is a NASA-funded program mainly for high school students that explores NASA science through art and highlights the need for and uses of art and visualizations in science. The project's aim is to motivate more diverse young people (especially African Americans) to consider Science, Technology, Engineering, and Mathematics (STEM) careers. The program offers intensive summer workshops at community youth centers, afterschool workshops at a local high school, a year-round internship for those who have taken part in one or more of our workshops, public and school outreach, and educator professional development workshops. By adding Art (fine art, graphic art, multimedia, design, and "maker/tinkering" approaches) to STEM learning, we wanted to try a unique combination of what's often now called the "STEAM movement" in STEM education. We've paid particular attention to highlighting how scientists and artists/tinkerers often collaborate, and why scientists need visualization and design experts. The program values the rise of the STEAM teaching concept, particularly that art, multimedia, design, and maker projects can help communicate science concepts more effectively. We also promote the fact that art, design, and visualization skills can lead to jobs and broader participation in science, and we frequently work with and showcase scientific illustrators and other science visualization professionals. This presentation will highlight the significant findings from our multi-year program.

  10. Toxicity assessment in marine sediment for the Terra Nova environmental effects monitoring program (1997-2010)

    Science.gov (United States)

    Whiteway, Sandra A.; Paine, Michael D.; Wells, Trudy A.; DeBlois, Elisabeth M.; Kilgour, Bruce W.; Tracy, Ellen; Crowley, Roger D.; Williams, Urban P.; Janes, G. Gregory

    2014-12-01

    This paper discusses toxicity test results on sediments from the Terra Nova offshore oil development. The Terra Nova Field is located on the Grand Banks approximately 350 km southeast of Newfoundland (Canada). The amphipod (Rhepoxynius abronius) survival and solid phase luminescent bacteria (Vibrio fischeri, or Microtox) assays were conducted on sediment samples collected from approximately 50 stations per program year around Terra Nova during baseline (1997), prior to drilling, and in 2000, 2001, 2002, 2004, 2006, 2008 and 2010 after drilling began. The frequency of toxic responses in the amphipod toxicity test was low. Of the ten stations that were toxic in environmental effects monitoring (EEM) years, only one (station 30(FE)) was toxic in more than one year and could be directly attributed to Terra Nova project activities. In contrast, 65 (18%) of 364 EEM samples were toxic to Microtox. Microtox toxicity in EEM years was not related to distance from Terra Nova drill centres or concentrations of >C10-C21 hydrocarbons or barium, the primary constituents of the synthetic-based drill muds used at Terra Nova. Of the variables tested, fines and strontium levels showed the strongest (positive) correlations with toxicity. Neither fines nor strontium levels were affected by drill cuttings discharge at Terra Nova, except at station 30(FE) (and that station was not toxic to Microtox). Benthic macro-invertebrate abundance, richness and diversity were greater in toxic than in non-toxic sediments. Therefore, Microtox responses indicating toxicity were associated with positive biological responses in the field. This result may have been an indirect function of the increased abundance of most invertebrate taxa in less sandy sediments with higher gravel content, where fines and strontium levels and, consequently, toxicity to Microtox were high; or chemical substances released by biodegradation of organic matter, where invertebrates are abundant, may be toxic to Microtox. Given

  11. Tourism Development Plan for Nova Lima, MG/BR: A Case Study

    Directory of Open Access Journals (Sweden)

    Porto Aluisio Finazzi

    2014-01-01

    Full Text Available The project called “Tourism Development Plan of Nova Lima, MG” was a labor required by the city of Nova Lima, through the Secretary of Municipal Tourism. The municipality of Nova Lima has numerous tourist attractions or potential for them attractive, and is developing a work of public policies aimed at structuring this activity. The objective of this project was to offer to its population, as well as the government and the private sector, the assurance of quality activity according to the international, national and state the assumptions referred to in the Municipal Tourism Plan. All work was developed by Scientific and Technical Research Data Collection, which took into consideration the participation of local stakeholders in the development of tourism through public hearings with the Section for Local Tourism, making use of Information from the Current Municipal Development Plan for Nova Lima and its Secretary of Tourism. We also note that the study was conducted in accordance with the guidelines and considerations of the Municipal Tourism Council (COMTUR of Nova Lima.

  12. Muon Neutrino Disappearance in NOvA with a Deep Convolutional Neural Network Classifier

    Science.gov (United States)

    Rocco, Dominick Rosario

    The NuMI Off-axis Neutrino Appearance Experiment (NOvA) is designed to study neutrino oscillation in the NuMI (Neutrinos at the Main Injector) beam. NOvA observes neutrino oscillation using two detectors separated by a baseline of 810 km; a 14 kt Far Detector in Ash River, MN and a functionally identical 0.3 kt Near Detector at Fermilab. The experiment aims to provide new measurements of $[special characters omitted]. and theta23 and has potential to determine the neutrino mass hierarchy as well as observe CP violation in the neutrino sector. Essential to these analyses is the classification of neutrino interaction events in NOvA detectors. Raw detector output from NOvA is interpretable as a pair of images which provide orthogonal views of particle interactions. A recent advance in the field of computer vision is the advent of convolutional neural networks, which have delivered top results in the latest image recognition contests. This work presents an approach novel to particle physics analysis in which a convolutional neural network is used for classification of particle interactions. The approach has been demonstrated to improve the signal efficiency and purity of the event selection, and thus physics sensitivity. Early NOvA data has been analyzed (2.74 x 1020 POT, 14 kt equivalent) to provide new best-fit measurements of sin2(theta23) = 0.43 (with a statistically-degenerate compliment near 0.60) and [special characters omitted]..

  13. Searching for Magnetar-powered Merger-novae from Short GRBS

    Science.gov (United States)

    Gao, He; Zhang, Bing; Lü, Hou-Jun; Li, Ye

    2017-03-01

    The merger of a double neutron star (NS–NS) binary may result in a rapidly rotating massive NS with an extremely strong magnetic field (i.e., a millisecond magnetar). In this case, the magnetic spin-down of the NS remnant provides an additional source of sustained energy injection, which would continuously power the merger ejecta. The thermal emission from the merger ejecta would give rise to a bright optical “magnetar-powered merger-nova.” In this work, we carry out a complete search for magnetar-powered merger-nova from a Swift short gamma-ray burst sample. We focus on short GRBs with extended emission or internal plateau, which may signify the presence of magnetars as the central engine. We eventually find three candidates of magnetar-powered merger-nova from the late observations of GRB 050724, GRB 070714B, and GRB 061006. With standard parameter values, the magnetar remnant scenario could well interpret the multi-band data of all three bursts, including the extended emission and their late chromatic features in the optical and X-ray data. The peak luminosities of these merger-novae reach several times {10}42 {erg} {{{s}}}-1, more than one order of magnitude brighter than the traditional “kilo-novae” with peak luminosity of ∼ {10}41 {erg} {{{s}}}-1. Intense, multi-color, late-time observations of short GRBs are encouraged to identify more merger-novae in the future.

  14. Superhumps in the Rarely Outbursting SU UMa-Type Dwarf Nova, HO Delphini

    CERN Document Server

    Kato, T; Moilanen, M; Yamaoka, H

    2003-01-01

    We observed the 1994, 1996 and 2001 outbursts of HO Del. From the detection of secure superhumps, HO Del is confirmed to be an SU UMa-type dwarf nova with a superhump period of 0.06453(6) d. Based on the recent observations and the past records, the outbursts of HO Del are found to be relatively rare, with the shortest intervals of superoutbursts being ~740 d. Among SU UMa-type dwarf novae with similar outburst intervals, the outburst amplitude (~5.0 mag) is unusually small. HO Del showed a rather rapid decay of the superhump amplitudes, and no regrowth of the amplitudes during the later stage, in contrast to the commonly observed behavior in SU UMa-type dwarf novae with long outburst intervals. We positively identified HO Del with a ROSAT X-ray source, and obtained a relatively large X-ray luminosity of 10^(31.1+/-0.2) erg/s. We also performed a literature survey of SU UMa-type dwarf novae, and presented a new set of basic statistics. The SU UMa-type dwarf novae with a brightening trend or with a regrowth of...

  15. Non-LTE Luminosity and Abundance Diagnostics of Classical Novae in X-rays

    CERN Document Server

    Németh, Péter

    2013-01-01

    Classical novae are significant sources of interstellar material, especially carbon, nitrogen and oxygen. These standard candles are only behind supernovae and $\\gamma$-ray bursts as the third brightest objects in the sky, and the most probable progenitors of type Ia supernovae. After a nova outburst the system enters into the constant bolometric luminosity phase and the nova maintains a stable hydrogen burning in the surface layers of the white dwarf. As the expanding shell around the nova attenuates, progressively deeper and hotter layers become visible. At the end of the constant bolometric luminosity phase, the hottest layers are exposed and novae radiate X-rays. This work uses the static, plane-parallel model atmosphere code TLUSTY to calculate atmospheric structure and SYNSPEC to calculate synthetic X-ray spectra. It was necessary to incorporate atomic data for the highest ionization stages of elements ranging from hydrogen to iron in both programs. Atomic data on energy levels, bound-free, bound-bound ...

  16. A near-infrared catalogue of the Galactic novae in the VVV survey area

    CERN Document Server

    Saito, R K; Angeloni, R; Catelan, M; Beamin, J C; Borissova, J; Dekany, I; Kerins, E; Kurtev, R; Mennickent, R E

    2013-01-01

    Near-IR data of Classical Novae contain useful information about the ejected gas mass and the thermal emission by dust formed during eruption, and provide independent methods to classify the objects according to the colour of their progenitors, and the fading rate and features seen after eruption. The VISTA Variables in the Via Lactea survey (VVV) is a near-IR ESO Public Survey mapping the MW bulge and southern plane. Data taken during 2010-2011 covered the entire area in the JHKs bands plus some epochs in Ks-band of the ongoing VVV variability campaign. We used the novae list provided by VSX/AAVSO catalogue to search for all objects within the VVV area. We used the VVV data to create a near-IR catalogue of the known Galactic novae in the 562 sq.deg. area covered by VVV. The VVV near-IR catalogue of novae contains JHKs photometry of 93 objects completed as of December 2012. We also checked in the ongoing VVV variability campaign for the light-curves of novae that erupted in the last years. VVV images can also...

  17. Proton capture reaction of 33S in nova V1065 Centauri

    Institute of Scientific and Technical Information of China (English)

    Luo Zhi-Quan; Zhang Jie; Long Jian-Hong

    2012-01-01

    Previous studies have shown that 33S(p,γ)34Cl is the most important reaction that affects the abundance of 33S in the product of nova nucleosynthesis.In this paper,a more accurate thermonuclear reaction rate of 33S(p,γ)34Cl in the nova is calculated based on the newly measured 34Cl nuclear resonance levels.The electron screening correction and the non-resonance and narrow-resonance contributions are considered.The calculations are also combined with the recent observational data of nova V1065 Centauri and show that the thermonuclear reaction rates of 33S(p,γ) 34Cl are significantly different in the improved method.Because these results can affect the isotopic ratio of sulfur in the nova ejecta significantly,we make an estimate of the values of 32S/33S and 33S/33S☉,which can be used as a diagnostic tool for the novae.

  18. Nuclear ashes and outflow in the eruptive star Nova Vul 1670

    CERN Document Server

    Kaminski, Tomasz; Tylenda, Romuald; Hajduk, Marcin; Patel, Nimesh A; Kraus, Alexander

    2015-01-01

    CK Vulpeculae was observed in outburst in 1670-16721, but no counterpart was seen until 1982, when a bipolar nebula was found at its location. Historically, CK Vul has been considered to be a nova (Nova Vul 1670), but a similarity to 'red transients', which are more luminous than classical nova and thought to be the result of stellar collisions, has re-opened the question of CK Vul's status. Red transients cool to resemble late M-type stars, surrounded by circumstellar material rich in molecules and dust. No stellar source has been seen in CK Vul, though a radio continuum source was identified at the expansion centre of the nebula. Here we report CK Vul is surrounded by chemically rich molecular gas with peculiar isotopic ratios, as well as dust. The chemical composition cannot be reconciled with a nova or indeed any other known explosion. In addition, the mass of the surrounding gas is too high for a nova, though the conversion from observations of CO to a total mass is uncertain. We conclude that CK Vul is ...

  19. Clearing the Gas from Globular Clusters & Dwarf Spheroidals with Classical Novae

    CERN Document Server

    Moore, Kevin

    2010-01-01

    Observations of the intra-cluster medium (ICM) in galactic globular clusters (GCs) show a systematic deficiency in ICM mass as compared to that expected from accumulation of stellar winds in the time available between galactic plane crossings. In this paper, we reexamine the original hypothesis of Scott and Durisen that hydrogen-rich explosions on accreting white dwarfs, classical novae (CNe), will sweep out the ICM from the cluster more frequently than galactic plane crossings. From the CNe rate and stellar mass-loss rate, this clearing mechanism predicts that ~ 0.03 M_sun should be present in 5x10^5 M_sun) GCs. We find that nova shells are effective at clearing the ICM in low-mass GCs (<= 10^5 M_sun), whereas higher-mass clusters may experience a quiescent time between novae long enough to prevent the next nova shell from escaping. The nova clearing mechanism will also operate in ultra-faint Milky Way satellites, where many upper limits on gas masses are available.

  20. Quark-Novae Ia in the Hubble diagram: Implications For Dark Energy

    CERN Document Server

    Ouyed, Rachid; Leahy, Denis; Staff, Jan E; Cassidy, Daniel T

    2013-01-01

    The accelerated expansion of the Universe was proposed through the use of Type-Ia SNe as standard candles. The standardization depends on an empirical correlation between the stretch/color and peak luminosity of the light curves. The use of Type Ia SN as standard candles rests on the assumption that their properties (and this correlation) do not vary with red-shift. We consider the possibility that the majority of Type-Ia SNe are in fact caused by a Quark-Nova detonation in a tight neutron-star-CO-white-dwarf binary system; a Quark-Nova Ia. The spin-down energy injected by the Quark Nova remnant (the quark star) contributes to the post-peak light curve and neatly explains the observed correlation between peak luminosity and light curve shape. We demonstrate that the parameters describing Quark-Novae Ia are NOT constant in red-shift. Simulated Quark-Nova Ia light curves provide a test of the stretch/color correlation by comparing the true distance modulus with that determined using SN light curve fitters. We d...

  1. Novas Fontes, Novas Versões: Contribuições do Acervo da Comissão Nacional da Verdade

    Directory of Open Access Journals (Sweden)

    Alessandra Sá Mello Costa

    2017-03-01

    Full Text Available Na área de estudos organizacionais, o interesse dos pesquisadores em utilizar fontes e acervos históricos em suas pesquisas cresce a cada dia (Rowlinson, Hassard, & Decker, 2014; Yates, 2014. Como forma de enriquecer e aprofundar a discussão sobre esse movimento, a presente pesquisa tem por objetivo refletir sobre possíveis contribuições das fontes reunidas, sistematizadas e produzidas pela Comissão Nacional da Verdade (CNV. Instituída para investigar as graves violações dos direitos humanos cometidas no regime da ditadura civil-militar brasileira, a CNV (a partir de seu acervo oferece aos pesquisadores das organizações novas versões dos fatos históricos, o que torna possível não só problematizar e rever versões históricas oficiais hegemônicas, mas também investigar fenômenos organizacionais sob outras perspectivas. Assim, após a descrição do processo de constituição e de composição do seu acervo documental, foram elencadas quatro avenidas de pesquisas iniciais: (a sobre o apoio e a participação da sociedade civil na constituição e manutenção do governo civil-militar brasileiro; (b sobre a formação de redes de agentes sociais envolvidos no processo de criação e de trabalho da CNV; (c sobre as relações de trabalho durante o período, como a atuação dos sindicatos ou as práticas de recursos humanos sob um regime autoritário; e (d sobre o tema da história e memória das empresas.

  2. On the narrow emission line components of the LMC novae 2004 (YY Dor) and 2009a

    CERN Document Server

    Mason, Elena

    2014-01-01

    We present early decline spectra of the two Large Magellanic Cloud novae: LMC 2004 (YY Dor) and LMC 2009a and discuss their spectral an line profile evolution with special emphasis on the existence and appearance of a sharp component. We show that the narrow component that characterizes the emission lines in the maximum spectra of nova LMC 2004 originates in the ejecta. The HeII 4686 A, narrow emission which appears at the onset of the nebular phase in both novae is somewhat controversial. Our observations suggest that the corresponding line forming region is physically separated from the rest of the ejecta (the broad line region) and environmentally different. However, the lack of late time observations covering the super-soft source (SSS) phase, the post-SSS phase and the quiescence state does not allow to securely establish any non-ejecta origin/contribution as, instead, in the case of U Sco and KT Eri.

  3. Expanding Pharmacists' Scope of Practice to Include Immunization in Nova Scotia

    Directory of Open Access Journals (Sweden)

    Beth O'Reilly

    2017-07-01

    Full Text Available On 10 December 2010 An Act to Amend Chapter 36 of the Acts of 2001, the Pharmacy Act (Bill 7 received Royal Assent in Nova Scotia, including an amendment that enabled an expanded scope of pharmacy practice. Expanding pharmacists' scope of practice came about from recommendations by various federal and provincial government bodies as an attempt to improve accessibility to health care and decrease costs. In 2013, pharmacists in Nova Scotia began administering the influenza vaccine as part of the publicly funded program in attempts to improve vaccine coverage rates. Preliminary evaluation in Nova Scotia has shown an increase in influenza vaccination coverage. Although pharmacist administration of influenza vaccination may improve vaccination coverage and reduce demand on physician time, there may be tension created among the professions, which needs to be addressed and managed.

  4. Superoutburst of a New Sub-Period-Minimum Dwarf Nova CSS130418 in Hercules

    Directory of Open Access Journals (Sweden)

    D. Chochol

    2015-02-01

    Full Text Available Multicolour photometry of a new dwarf nova CSS130418 in Hercules, which underwent superoutburst on April 18, 2013, allow to classified it as a WZ Sge-type dwarf nova. The phase light curves for different stages of superoutburst are presented. The early superhumps were used to determine the orbital period Porb = 64.84(1 minutes, which is shorter than the period minimum ~78 minutes for normal hydrogen-rich cataclysmic variables. We found the mean period of ordinary superhumps Psh = 65.559(1 minutes. The quiescent spectrum is rich in helium, showing double peaked emissionlines of H I and He I from accretion disk, so the dwarf nova is in a late stage of stellar evolution.

  5. The Effects of Thermonuclear Reaction Rate Variations on Nova Nucleosynthesis A Sensitivity Study

    CERN Document Server

    Iliadis, C; José, J; Starrfield, S; Tupper, P; Iliadis, Christian; Champagne, Art; Jose, Jordi; Starrfield, Sumner; Tupper, Paul

    2002-01-01

    We investigate the effects of thermonuclear reaction rate uncertainties on nova nucleosynthesis. One-zone nucleosynthesis calculations have been performed by adopting temperature-density-time profiles of the hottest hydrogen-burning zone (i.e., the region in which most of the nucleosynthesis takes place). We obtain our profiles from 7 different, recently published, hydrodynamic nova simulations covering peak temperatures in the range from Tpeak=0.145-0.418 GK. For each of these profiles, we individually varied the rates of 175 reactions within their associated errors and analyzed the resulting abundance changes of 142 isotopes in the mass range below A=40. In total, we performed 7350 nuclear reaction network calculations. We use the most recent thermonuclear reaction rate evaluations for the mass ranges A=1-20 and A=20-40. For the theoretical astrophysicist, our results indicate the extent to which nova nucleosynthesis calculations depend on presently uncertain nuclear physics input, while for the experimenta...

  6. Modelling the synchrotron light curves in recurrent novae V745 Scorpii and RS Ophiuchi

    CERN Document Server

    Kantharia, N G; Roy, N; Anupama, G C; Chitale, A; Ishwara-Chandra, C; Prabhu, T P; Ashok, N M; Banerjee, D P K

    2015-01-01

    In this paper, we present the synchrotron light curve at 610 MHz from the recurrent nova V745 Sco following its outburst on 6 February 2014. The system has been detected and periodically monitored with the Giant Metrewave Radio Telescope (GMRT) since 9 February 2014 as part of the Galactic Nova with GMRT (GNovaG) project. The light curves are well fit by a model of synchrotron emitting region obscured by foreground thermal gas which eventually becomes optically thin to the low GMRT frequencies. We present the model fit to the 2014 data on V745 Sco and discuss it alongwith the model fit to the 1.4 GHz data of the recurrent nova RS Ophiuchi following its outburst in 1985.

  7. A Far Ultraviolet Spectroscopic Analysis of the Old Nova Q Cygni

    Science.gov (United States)

    Kolobow, Craig; Sion, E. M.

    2011-01-01

    Q Cygni (Nova Cygni 1876) is one of the oldest old novae with a long orbital period of 10.08 hours and spectroscopic peculiarities in the optical including the presence of variable wind outflow revealed by optical P Cygni profiles in the He I lines and Halpha (Kafka et al.2003). There has never been a far UV spectroscopic analysis of this system. Therefore, we have carried out a synthetic spectral analysis of a far ultraviolet IUE archival spectrum of Q Cygni using our optically thick, steady state, accretion disk models and model white dwarf photospheres. We report the results of our spectroscopic analysis and compare the physical parameters we derive with those of other old novae. We gratefully acknowledge the support of this by NSF grant 0807892 to Villanova University.

  8. The 2010 nova outburst of the symbiotic Mira V407 Cyg

    CERN Document Server

    Munari, U; Ashok, N M; Banerjee, D P K; Valisa, P; Milani, A; Siviero, A; Dallaporta, S; Castellani, F

    2010-01-01

    The nova outburst experienced in 2010 by the symbiotic binary Mira V407 Cyg has been extensively studied at optical and infrared wavelengths with both photometric and spectroscopic observations. This outburst, reminiscent of similar events displayed by RS Oph, can be described as a very fast He/N nova erupting while being deeply embedded in the dense wind of its cool giant companion. The hard radiation from the initial thermonuclear flash ionizes and excites the wind of the Mira over great distances (recombination is observed on a time scale of 4 days). The nova ejecta is found to progressively decelerate with time as it expands into the Mira wind. This is deduced from line widths which change from a FWHM of 2760 km/s on day +2.3 to 200 km/s on day +196. The wind of the Mira is massive and extended enough for an outer neutral and unperturbed region to survive at all outburst phases.

  9. A bossa nova e a influência do blues, 1955-1964

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    Bryan McCann

    2010-06-01

    Full Text Available Este artigo considera as conexões entre blues e bossa nova, pouco reconhecidas na literatura sobre bossa nova mas muito importantes para o desenvolvimento do estilo. Analisando as gravações do circuito samba-jazz em Copacabana nas décadas de 1950 e 1960, o artigo traz à luz uma prática de blues, tanto na estrutura de doze compassos como na utilização da escala blues como matéria de improviso, bastante comum naquela época. O artigo explica o papel de figuras-chaves como Booker Pittman, Moacir Santos e Paulo Moura na transmissão de uma influência do blues no Rio de Janeiro e os efeitos dessa influência na bossa nova.

  10. AMMONIZATION IN THE PRODUCTION RESIDUE OF FODDER SEEDS IN THE PERFORMANCE AND BIOMETRY OF LAMBS AMONIZAÇÃO DO RESÍDUO DA PRODUÇÃO DE SEMENTES DE FORRAGEM NO DESEMPENHO E BIOMETRIA DE CORDEIROS

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    Gustavo Rezende Siqueira

    2009-09-01

    Full Text Available In order to evaluate the effect of ammonization in the production residue of Brachiaria brizantha seeds in the performance and in vivo biometric measurements of sheep, 19 Santa Inês lambs (females and non-castrated males were used, with initial weight of 15kg, confined in individual cages until reaching 28kg. Animals were arranged into two groups, receiving isoenergetic and isoproteic diets with 40:60 volumous:concentrate ratio, being diet 1 (D1 made up with non-treated volumous with urea + addiction of urea in concentrate and diet 2 (D2 with treated volumous with addiction of 2% urea in MS + concentrate without urea. Dry matter consumption was similar between diets and sexes (0.85 kg/day, 3.28%/BW e 73.15 g/kg0,75/day; however, the remaining performance parameters were affected by the different sexes of animals. There was not interaction between diet and sex in biometric measurements; however, body length was higher for females (66.50 cm compared to males (61.12 cm. We conclude that the effect of ammonization in diet volumous did not affect performance and biometric measurements of sheep terminated in confinement, being that some changes occurred due to the different sexes of the animals.

    KEY WORDS: Chemical treatment, nutritional value, sheep, urea, volumous.
    Para avaliar o efeito da amonização no resíduo da produção de sementes de Brachiaria brizantha no desempenho e nas medidas biométricas in vivo de ovinos, foram utilizados dezenove cordeiros (machos não castrados e fêmeas da raça Santa Inês, com peso inicial de quinze kg, confinados em gaiolas individuais até atingirem 28 kg. Distribuíram-se os animais em dois grupos, recebendo dietas isoenergéticas e isoproteicas com relação volumoso:concentrado 40:60, sendo a dieta 1 (D1 constituída de volumoso não amonizado + inclusão de ureia no concentrado e D2 com volumoso tratado com inclusão de 2% de ureia na MS + concentrado sem ureia. O consumo de mat

  11. Near-infrared studies of V2944 Ophiuchi (Nova Ophiuchi 2015)

    Science.gov (United States)

    Srivastava, Mudit K.; Banerjee, D. P. K.; Ashok, N. M.; Venkataraman, V.; Sand, D.; Diamond, T.

    2016-10-01

    We present multi-epoch near-infrared observations of Nova Ophiuchi 2015 which was discovered during outburst in March 2015. This nova showed a few special properties viz. (i) it displayed an unusual prolonged flat-top light curve which does not easily fit into known classes of nova light curves, (ii) it showed evidence for possessing an evolved secondary in the outbursting binary system, and (iii) it made a rare reverse hybrid transition from the He/N class to Fe II class early during its outburst. The present studies focus on the spectroscopic evolution of the object around maximum light and early decline. We show that there was a unique, rapid strengthening and decline in the He 1.0831, 2.0581 μm line strengths during this stage, wherein the nova combined the traits of both the He/N and Fe II classes. Possible causes for this behaviour are discussed. The relative strengths of the Lyβ fluoresced O I 0.8446, 1.1287 μm lines are used to estimate the reddening to the nova. A recombination Case B analysis of the early spectra is used to set constraints on the electron density and emission measure, and a later time spectrum when the ejecta were optically thin is used to estimate the ejecta mass to be (0.95-1.9) × 10-4 M⊙. Power-law fits made to study the evolution of the continuum, show a fairly constant slope which differs from the trend generally expected during a nova's evolution viz. beginning with a blackbody and evolving to a free-free distribution at later stages.

  12. VizieR Online Data Catalog: New Dwarf novae in SDSS, GALEX and astrom. cat. (Wils+, 2010)

    Science.gov (United States)

    Wils, P.; Gansicke, B. T.; Drake, A. J.; Southworth, J.

    2015-07-01

    Here, we cross-match a number of large surveys to find faint outbursting dwarf novae, and make use of CRTS light curves to compare the properties of the previously known dwarf novae, those identified spectroscopically by SDSS, and the ones discovered in this paper. (3 data files).

  13. Four unusual novae observed in Torun: V2362 Cyg, V2467 Cyg, V458 Vul, V2491 Cyg

    CERN Document Server

    Ragan, E; Tomov, T; Dimitrow, W; Fagas, M; Kwiatkowski, T; Schwarzenberg-Czerny, A; Buil, Ch; Swierczynski, E; Brozek, T; Cikala, M; Czart, K; Fidos, A; Frackowiak, S; Galan, C; Karska, A; Klosinska, M; Lewandowski, M; Radomski, T; Rozanski, P; Wiecek, M; Wychudzki, P; Zajczyk, A; Zielinska, M

    2010-01-01

    We present photometric and spectral observation for four novae: V2362 Cyg, V2467 Cyg, V458 Vul, V2491 Cyg. All objects belongs to the "fast novae" class. For these stars we observed different departures from a typical behavior in the light curve and spectrum.

  14. Modelling sea ice formation in the Terra Nova Bay polynya

    Science.gov (United States)

    Sansiviero, M.; Morales Maqueda, M. Á.; Fusco, G.; Aulicino, G.; Flocco, D.; Budillon, G.

    2017-02-01

    Antarctic sea ice is constantly exported from the shore by strong near surface winds that open leads and large polynyas in the pack ice. The latter, known as wind-driven polynyas, are responsible for significant water mass modification due to the high salt flux into the ocean associated with enhanced ice growth. In this article, we focus on the wind-driven Terra Nova Bay (TNB) polynya, in the western Ross Sea. Brine rejected during sea ice formation processes that occur in the TNB polynya densifies the water column leading to the formation of the most characteristic water mass of the Ross Sea, the High Salinity Shelf Water (HSSW). This water mass, in turn, takes part in the formation of Antarctic Bottom Water (AABW), the densest water mass of the world ocean, which plays a major role in the global meridional overturning circulation, thus affecting the global climate system. A simple coupled sea ice-ocean model has been developed to simulate the seasonal cycle of sea ice formation and export within a polynya. The sea ice model accounts for both thermal and mechanical ice processes. The oceanic circulation is described by a one-and-a-half layer, reduced gravity model. The domain resolution is 1 km × 1 km, which is sufficient to represent the salient features of the coastline geometry, notably the Drygalski Ice Tongue. The model is forced by a combination of Era Interim reanalysis and in-situ data from automatic weather stations, and also by a climatological oceanic dataset developed from in situ hydrographic observations. The sensitivity of the polynya to the atmospheric forcing is well reproduced by the model when atmospheric in situ measurements are combined with reanalysis data. Merging the two datasets allows us to capture in detail the strength and the spatial distribution of the katabatic winds that often drive the opening of the polynya. The model resolves fairly accurately the sea ice drift and sea ice production rates in the TNB polynya, leading to

  15. Ciencias contábeis, novos rumos , novas diretrizes curriculares

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    Patricia Dantas Trajano

    2009-09-01

    Full Text Available A nova Lei de Diretrizes e Bases da Educação Nacional, Lei n"9.394, de 20 de dezembro de 1996, em seu artigo 43, enfatiza que a educação superior tem por finalidade precípua a formação de profissionais aptos para inserção no mercado de trabalho e em condições de participarem ativamente do desenvolvimento da sociedade brasileira. Prevê, ainda, o incentivo a pesquisa, a educação continuada, assim como a promoção da divulgação de conhecimentos culturais, científicos e técnicos que constituam patrimônio da humanidade. O inciso II do artigo 53 da mesma Lei concede autonomia as Instituições de Ensino Superior (IES para "fixar os currículos dos seus cursos e programas, observadas as diretrizes gerais pertinentes", o que oferece as IES uma maior flexibilidade na elaboração de seu currículo pleno. A Resolução n2 03/92, do Conselho Federal de Educação, fixa, ate o momento, os mínimos de conteúdo e de duração do curso de graduação em Ciências Contábeis vigentes no pals. Estabelece que o currículo pleno das IES deva definir o perfil profissional a ser formado, em função das atribuições legais que lhe serão conferidas, das peculiaridades e necessidades da região em que as IES se encontram, de suas naturezas e características próprias. O currículo pleno deve ser dividido por disciplinas ou outras atividades curriculares obrigatórias eletivas, nas seguintes categorias de conhecimentos: Categoria I - Conhecimentos de Formação Geral de natureza humanística e social; Categoria II - Conhecimentos de Formação Profissional; Categoria III - Conhecimentos ou Atividades de Formação.

  16. ENSINO MÉDIO ARTICULADO AO ENSINO PROFISSIONALIZANTE: NOVAS PERSPECTIVAS

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    S. H. S. L. M. Freire

    2012-05-01

    Full Text Available Neste artigo pretendemos discutir sobre a nova proposta do Ensino Médio articulado ao Ensino profissionalizante, nas instituições SESI e SENAI na cidade de Mossoró/RN. Essa proposta tem por finalidade proporcionar a formação integral, alicerçada nas dimensões do trabalho, ciência e cultura e ampliar as possibilidades de inserção do cidadão na vida produtiva e social, bem como dar continuidade ao seu itinerário formativo, contribuindo para a formação continuada e permanente do aluno. Dessa maneira, objetivamos com esse estudo analisar as contribuições dessa articulação para ensino - aprendizagem do aluno e as possibilidades de construção de novos conhecimentos. O estudo fundamenta-se em documentos como referenciais normativos, pedagógico, operacionais e financeiros nacionais para a articulação da educação básica do SESI com a educação profissional do SENAI (2006, relatório de map