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Sample records for novas idades k-ar

  1. Algumas idades Rb-Sr e K-Ar de rochas granitóides da região de Vilarinho da Castanheira-Foz do Sabor (Carrazeda de Anciães-Nordeste de Portugal)

    OpenAIRE

    Silva, Antero Ferreira da; KAWASHITA,KOJI

    2005-01-01

    Neste trabalho apresentam-se algumas determinações isotópicas Rb/Sr e K/Ar de idades absolutas em rochas granitóides do antiforma de Alijó-Carviçais, correspondente à região es-sudeste de Carrazeda de Anciães (Vilarinho da Castanheira-Foz do Sabor). A rocha total de duas amostras dos granitos de Castedo-Cabanas de Cima e Zêdes-Cabeça Boa-Especiarias, indiferenciados localmente, proporcionaram as idades convencionais Rb/Sr de 361.1±23.8 e 404.7±22.3M.a., com razão inicial (87Sr/86S...

  2. Degeneração macular relacionada à idade: novas perspectivas Age-related macular degeneration: new perspectives

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    Marcio Bittar Nehemy

    2006-12-01

    Full Text Available A degeneração macular relacionada à idade (DMRI é a principal causa de cegueira legal em indivíduos acima de 50 anos de idade. Embora estudos recentes tenham mostrado que o fator genético é significativo, a patogênese da degeneração macular relacionada à idade permanece obscura, e os fatores de risco não estão ainda completamente estabelecidos. Estudos multicêntricos randomizados, publicados nos últimos anos, demonstraram que uma combinação de vitaminas e minerais é eficaz na redução do risco de desenvolvimento de neovascularização e de progressão para os estágios mais avançados da degeneração macular relacionada à idade. De maneira análoga, a terapia fotodinâmica (PDT e a terapia antiangiogênica também tiveram sua eficácia comprovada no tratamento de membrana neovascular coroideana subfoveal associada à degeneração macular relacionada à idade. Ambas reduzem o risco de perda de visão e, eventualmente, permitem melhora temporária da acuidade visual. Outras modalidades de tratamento, tais como fotocoagulação a laser, remoção cirúrgica da membrana e termoterapia transpupilar (TTT, podem beneficiar apenas um pequeno subgrupo de pacientes. Uma melhor compreensão dos mecanismos fisiopatológicos e dos eventos moleculares nas diversas fases da doença deverão propiciar, em futuro próximo, melhores estratégias para o controle e tratamento da degeneração macular relacionada à idade.Age-related macular degeneration (ARMD is a major source of legal blindness in individuals older than 50 years. Even though recent reports suggest that genetics plays an important role, its pathogenesis remains puzzling and the risk factors for its occurrence are not completely established. Vitamin and mineral supplementation reduced the risk of development of choroidal neovascularization (CNV or progression to the most advanced stages of age-related macular degeneration. Photodynamic therapy (PDT and antiangiogenic therapy

  3. Terceira idade: nova identidade, reinvenção da velhice ou experiência geracional? Third age: new identity, reformulation of the old age or generational experience?

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    Luna Rodrigues Freitas Silva

    2008-01-01

    Full Text Available Este artigo trata das inovações acerca dos modos e das experiências de envelhecer que se vêm configurando nos últimos anos. Hábitos, imagens, crenças e condutas atreladas ao envelhecimento vêm-se alterando de forma significativa, determinando o surgimento do que se convenciona chamar de experiência da terceira idade. Mas, ainda que represente inovação e, sob muitos aspectos, seja descrita como uma reformulação extremamente positiva das possibilidades de envelhecer, o surgimento da terceira idade gera também questionamento e debate. Para compreender o estatuto desta experiência que surge no cenário contemporâneo, procederemos a um mapeamento da discussão acerca da terceira idade na literatura especializada, mais especificamente no que se refere a seu caráter de inovação em relação à identidade da velhice. Três hipóteses se destacam nesta análise: a primeira sugere que a terceira idade pode ser entendida como uma nova identidade, autônoma e diferenciada da identidade da velhice; a segunda, que seu surgimento pode ser compreendido como uma negação social da velhice propriamente dita; e, finalmente, a terceira hipótese supõe que as características da terceira idade são tributárias da experiência geracional de determinado grupo social. As principais hipóteses de entendimento da terceira idade são apresentadas e discutidas tendo em vista as possibilidades de criação, diversificação e inovação da experiência subjetiva.This paper deals with innovations on the ways and on the experience of aging set up in recent years. Habits, images, beliefs and behaviors related to aging have changed determining the emergence of what is usually called the third age experience. But although it represents innovation and, in many ways, is described as a very positive reformulation of the possibilities of aging, the emergence of the third age also generates questioning and debate. In order to understand the status of this

  4. 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

  5. Combined K-Ar and 40Ar/39Ar dating of the upper Jaramillo reversal

    Science.gov (United States)

    Guillou, Herve; Carracedo, Juan Carlos; Kissel, Catherine; Laj, Carlo; Nomade, Sebastien; Perez Torrado, Francisco Jose; Rodriguez Gonzalez, Alejandro; Wandres, Camille

    2013-04-01

    The Jaramillo subchron was first evidenced in 1966 (Doell and Dalrymple) through the Rhyolotic domes of the Valles Caldera, New Mexico (USA). 40Ar/39Ar studies achieved by Spell et McDougall (1992), Spell et Harrison (1993), Izett and Obradovich (1994) and Singer et al. (1994) defined the base of this subchron at 1053±6 ka, and the ceiling at 986±5 ka. Channell et al. (2009) delimited the age of the Jaramillo subchron by astronomic calibration (base 1071 ka, top 990 ka). To provide additional absolute ages on this geomagnetic period, which is critical to improve our knowledge of the earth magnetic field behaviour, we have carried out a study combining paleomagnetism and isotopic dating of a lava sequence from Tenerife island. This sequence of basaltic lava flows is some 500 m thick. The first 400 m present, based on field magnetometer measurements, normal polarity lavas, with dykes of normal and reverse polarity, passing at the top to reverse polarity lavas. Preliminary K-Ar ages bracketed this sequence between 1018 ± 18 ka and 978 ± 17 ka. Therefore, the upper Jaramillo reversal at least appeared to be potentially recorded in this sequence. A more detailed paleomagnetic study was then carried out to more precisely delimit the reversal itself (see Laj et al., session EMRP3.4). We have undertaken 40Ar/39Ar incremental heating and unspiked K-Ar experiments on groundmass from four transitionally magnetized flows. The first transitional flow is K-Ar dated at 993 ± 18 ka and 40Ar/39Ar dated at 991 ± 13 ka, the second at 981 ± 17 ka (K-Ar) and 1000 ± 13 ka (40Ar/39Ar), the third at 950 ± 17 ka (K-Ar) and 1000 ± 8 ka (40Ar/39Ar) and the fourth at 984 ± 17 ka (K-Ar) and 977 ± 12 (40Ar/39Ar). 40Ar/39Ar ages and K-Ar ages (relative to FCT 28.02 Ma) are indistinguishable at 2σ. The age of the upper boundary of the Jaramillo event calculated combining 40Ar/39Ar ages and K-Ar ages is 992 ± 6 ka, in agreement with previous estimates.

  6. K-Ar ages for the Yahazudake volcanic rocks from southwest Kyushu, Japan; Kyushu nanseibu yahazudake kazanganrui no K-Ar nendai

    Energy Technology Data Exchange (ETDEWEB)

    Yokose, H.; Kikuchi, W. [Kumamoto Univ. (Japan)] Nagao, K. [Okayama Univ. (Japan)264000] Kodama, K. [Kochi Univ. (Japan)

    1998-05-05

    Many volcanic rocks, seemed to be erupted during the period from the Pliocene epoch to the Pleistocene epoch, are distributed abounding in Kyushu, Japan. In this study, K-Ar ages determination about the 4 samples which represents the Hisatsu volcanic rocks distributed around Yahazudake and rhyolite distributed in Gesujima placed in the southernmost extremity of Amakusa Shimojima, was conducted. And consideration of time/space distribution of the Hisatsu volcanic rocks upon collecting the data which were reported until now and the data obtained by the present K-Ar age determination, was done. In the result of the present measurement, the absolute age of the Hisatsu volcanic rocks distributed around Minamata-shi became clear. I was clarified that Yahazudake volcanic rocks consisted of andesite, which is comparatively lacking in potassium, were formed during about 100 thousand years from 1.98 to 2.08 Ma, and Ontake volcanic rocks which exists for the bottom erupted at about 2.15 Ma. And, the age value of 2.89 Ma was obtained from Ushibuka rhyolite distributed in Gesujima. 35 refs., 4 figs., 3 tabs.

  7. K/AR dating of clinoptilolite, mordenite, and associated clays from Yucca Mountains, Nevada

    Energy Technology Data Exchange (ETDEWEB)

    WoldeGabriel, G.

    1993-07-01

    Zeolites are abundant in the geologic record in both continental and marine environments. The purpose of the present study is to evaluate the utility of K-bearing zeolites for dating by the K/Ar method to determine the time of zeolite diagenesis at Yucca Mountain, Nevada (Fig. 1). At Yucca Mountain, K-rich clinoptilolite and possibly mordenite are the only potentially K/Ar dateable secondary minerals present in the zeolite-rich tuffs except for some illite/smectites ({ge}10% illite layers) associated with these minerals. Direct dating of K-rich clinoptilolite, the most abundant zeolite in the altered tuffs, is important to delineate zeolite chronology as part of the site characterization of Yucca Mountain.

  8. Discordant K-Ar and young exposure dates for the Windjana sandstone, Kimberley, Gale Crater, Mars

    Science.gov (United States)

    Vasconcelos, P. M.; Farley, K. A.; Malespin, C. A.; Mahaffy, P.; Ming, D.; McLennan, S. M.; Hurowitz, J. A.; Rice, Melissa S.

    2016-10-01

    K-Ar and noble gas surface exposure age measurements were carried out on the Windjana sandstone, Kimberley region, Gale Crater, Mars, by using the Sample Analysis at Mars instrument on the Curiosity rover. The sandstone is unusually rich in sanidine, as determined by CheMin X-ray diffraction, contributing to the high K2O concentration of 3.09 ± 0.20 wt % measured by Alpha-Particle X-ray Spectrometer analysis. A sandstone aliquot heated to 915°C yielded a K-Ar age of 627 ± 50 Ma. Reheating this aliquot yielded no additional Ar. A second aliquot heated in the same way yielded a much higher K-Ar age of 1710 ± 110 Ma. These data suggest incomplete Ar extraction from a rock with a K-Ar age older than 1710 Ma. Incomplete extraction at 900°C is not surprising for a rock with a large fraction of K carried by Ar-retentive K-feldspar. Likely, variability in the exact temperature achieved by the sample from run to run, uncertainties in sample mass estimation, and possible mineral fractionation during transport and storage prior to analysis may contribute to these discrepant data. Cosmic ray exposure ages from 3He and 21Ne in the two aliquots are minimum values given the possibility of incomplete extraction. However, the general similarity between the 3He (57 ± 49 and 18 ± 32 Ma, mean 30 Ma) and 21Ne (2 ± 32 and 83 ± 24 Ma, mean 54 Ma) exposure ages provides no evidence for underextraction. The implied erosion rate at the Kimberley location is similar to that reported at the nearby Yellowknife Bay outcrop.

  9. K-Ar age constrains on chemically weathered granitic basement rocks (saprolites) in Scandinavia

    Science.gov (United States)

    Margreth, Annina; Fredin, Ola; Viola, Giulio; Knies, Jochen; Sørlie, Ronald; Lie, Jan-Erik; Margrethe Grandal, Else; Zwingmann, Horst; Vogt, Christoph

    2017-04-01

    Remnants of in-situ weathered bedrock, saprolite, are found in several locations in Scandinavia. Saprolites contain important information about past climate conditions and landscape evolution, although their age and genesis are commonly difficult to constrain. It is generally thought that clay-poor, coarse-grained (arêne) saprolites, mostly occurring as thin regolith blankets or in larger outcrops, formed in temperate climate during the Cenozoic, whereas clay-rich (argillic) saprolites, commonly restricted to small, fracture-bounded outcrops, formed in (sub-)tropical climate during the Mesozoic. Recent methodological and conceptual advances in K-Ar dating of illite-bearing fault rocks have been applied to date clay-rich saprolites. To test the K-Ar dating technique for saprolites, we first selected an offshore site in the Viking Graben of the North Sea, where weathered and fractured granitic basement highs have been drilled during petroleum exploration, and an abandoned kaolin mine in Southern Sweden. Both targets provide independent age control through the presence of overlying Mesozoic sedimentary rocks. Clay-rich saprolites occurring in fractured basement rocks were additionally sampled in a joint valley landscape on the southwestern coast of Norway, which can be regarded as the possible onland correlative to the offshore basement high. In order to offer a sound interpretation of the obtained K-Ar ages, the mineralogical and chemical composition of the saprolites requires a thorough characterization. Scanning electron microscopy of thin sections, integrated by XRD and XRF analysis, reveals the progressive transformation of primary granitic rock minerals into secondary clay minerals. The authigenesis of illite is particularly important to understand, since it is the only K-bearing clay mineral that can be dated by the K-Ar method. K-feldspars and mica are the common primary K-bearing minerals, from which illite can be formed. While progressive leaching of

  10. Application of K-Ar Dating to the Chronology of Young Volcanic Centers

    Science.gov (United States)

    Lanphere, M. A.

    2003-12-01

    K-Ar dating and a derivative technique, 40Ar/39Ar dating, are methods of high-precision chronology applicable to young volcanic centers. Cascade volcanoes studied in detail by several USGS volcanologists, Duane Champion paleomagetist, and me include Mt. Baker, WA; Mt. Rainier, WA; Mt. Adams, WA; Mt. Hood, OR; Crater Lake, OR; and Medicine Lake, CA. For Mt. Adams using detailed geologic mapping by Hildreth and Fierstein and 74 K-Ar ages for 63 mapped units, Hildreth and Lanphere established a detailed chronology for the stratovolcano. Good agreement has been achieved for K-Ar ages and 40Ar/39Ar ages of rocks from Mt. Adams as young as 36 ka. A similar detailed chronology has been established for other Cascade volcanoes using andesites, in particular. These chronologies often take 10 years or more to develop. Major advantages of the 40Ar/39Ar technique are the ability to work with small sample sizes and the possibility to push the technique to very young ages. The Campanian Ignimbrite erupted from the Campi Flegrei crater near Naples, Italy is an example of the use of small samples. Nine incremental-heating ages were determined on samples of sanidine ranging in size from 47 mg to 67 mg. These samples yielded ages for the Campanian Ignimbrite ranging from 37.1 +/- 0.75 ka to 39.5 +/- 0.62 ka and averaging 38.1 +/- 0.8 ka. Other workers have proposed 40Ar/39Ar ages for the Campanian Ignimbrite of 37.1 +/- 0.4 ka and 39.3 +/- 0.1 ka. An example of the use of 40Ar/39Ar dating of very young samples is the Christian Era (CE) age of the Vesuvius eruption of year 79. Eight packets of sanidine weighing 213-296 mg from two localities, Casti Amanti in Pompeii and Villa Poppea in nearby Oplontis, yielded a weighted-mean incremental-heating age of 1924 +/- 66 years. The known age for the CE 79 eruption of Vesuvius is 1924 years. Earlier studies of Vesuvius by other workers yielded an 40Ar/39Ar age for the Villa Poppea locality of 1922 +/- 72 years.

  11. Preliminary K/Ar geochronology of the Crater Basalt volcanic field (CBVF, northern Patagonia

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    Z. Pécskay

    2007-03-01

    Full Text Available The Crater Basalt volcanic field is one of the Quaternary intraplate basaltic fields in northern Patagonia. A systematic geological, volcanological and geochronological study of CBVF indicates a multistage history of eruptions of basaltic volcanoes. K/Ar dating, using whole rock samples shows that the measured analytical ages are fully consistent with the available stratigraphic control. The radiometric ages fall into three distinct, internally consistent age groups, which give evidence that there were at least three major episodes of volcanic activity, at about 1.0 Ma, 0.6 Ma and 0.3 Ma ago. The age differences appear to be just significant, even although less than 10 % radiogenic argon was found in the isotope analysis of whole rock samples.

  12. Preliminary K/Ar geochronology of the Crater Basalt volcanic field (CBVF, northern Patagonia

    Directory of Open Access Journals (Sweden)

    Z. Pécskay

    2007-11-01

    Full Text Available The Crater Basalt volcanic field is one of the Quaternary intraplate basaltic fields in northern Patagonia. A systematic geological, volcanological and geochronological study of CBVF indicates a multistage history of eruptions of basaltic volcanoes. K/Ar dating, using whole rock samples shows that the measured analytical ages are fully consistent with the available stratigraphic control. The radiometric ages fall into three distinct, internally consistent age groups, which give evidence that there were at least three major episodes of volcanic activity, at about 1.0 Ma, 0.6 Ma and 0.3 Ma ago. The age differences appear to be just significant, even although less than 10 % radiogenic argon was found in the isotope analysis of whole rock samples.El campo volcánico del Basalto Cráter (CVBC constituye uno de los campos basálticos cuaternarios de intraplaca de la Patagonia septentrional. El estudio sistemático de la geología, volcanología y geocronología del CVBC muestra una historia eruptiva multiepisódica de volcanes basálticos. Las dataciones K-Ar realizadas sobre roca total son coherentes con el control estratigráfico. Las edades obtenidas para el Basalto Cráter permiten distinguir tres episodios diferentes, pero individualmente coherentes, de actividad volcánica, ocurridos hace ~1,0 Ma; 0,6 Ma y 0,3 Ma. Las diferencias de edad parecen ser significativas, aún cuando el contenido de argón radiogénico determinado en los análisis de roca total resultó menor al 10 %.

  13. Conversion of K-Ar dates with modern constants : implications for recalculation of dates reported in Kawano and Ueda using constants reported by Steiger and Jager

    OpenAIRE

    Iwata, Naoyoshi

    2013-01-01

    This report describes details of a procedure used to convert from K-Ar dates with old constants reported in the relevant literature to K-Ar dates with modern decay constants and the isotopic ratio of potassium reported by Steiger and Jager. Nearly 300 K-Ar dates published by Kawano and Ueda in the 1960s have been recalculated using this procedure. These data are useful for comparing dates reported by Kawano and Ueda to recently obtained K-Ar dates reported by others.

  14. K-Ar geochronology of the late cenozoic volcanic rocks of the Cordillera Occidental, southernmost Peru

    Science.gov (United States)

    Tosdal, Richard M.; Farrar, Edward; Clark, Alan H.

    1981-05-01

    Twenty-four K-Ar radiometric ages are presented for late Cenozoic continental volcanic rocks of the Cordillera Occidental of southernmost Perú (lat. 16° 57'-17° 36'S). Rhyodacitic ignimbrite eruptions began in this transect during the Late Oligocene and continued episodically through the Miocene. The development of andesitic-dacitic strato volcanoes was initiated in the Pliocene and continues to the present. The earliest ignimbrite flows (25.3-22.7 Ma) are intercalated in the upper, coarsely-elastic member of the Moquegua Formation and demonstrate that this sedimentary unit accumulated in a trough, parallel to Andean tectonic trends, largely in the Oligocene. More voluminous ash-flow eruptions prevailed in the Early Miocene (22.8-17.6 Ma) and formed the extensively preserved Huaylillas Formation. This episode was coeval with a major phase of Andean uplift, and the pyroclastics overlie an erosional surface of regional extent incised into a Paleogene volcano-plutonic arc terrain. An age span of 14.2-8.9 Ma (mid-Late Miocene) is indicated for the younger Chuntacala Formation, which again comprises felsic ignimbrite flows, largely restricted to valleys incised into the pre-Huaylillas Formation lithologies, and, at lower altitudes, an extensive aggradational elastic facies. The youngest areally extensive ignimbrites, constituting the Sencca Formation, were extruded during the Late Miocene. In the earliest Pliocene, the ignimbrites were succeeded by more voluminous calcalkaline, intermediate flows which generated numerous large and small stratovolcanoes; these range in age from 5.3 to 1.6 Ma. Present-day, or Holocene, volcanism is restricted to several large stratovolcanoes which had begun their development during the Pleistocene (by 0.7 Ma). The late Oligocene/Early Miocene (ca. 22-23 Ma) reactivation of the volcanic arc coincided with a comparable increase in magmatic activity throughout much of the Cordilleras Occidental and Oriental of the Central Andes.

  15. Preliminary assessment of clinoptilolite K/Ar results from Yucca Mountain, Nevada, USA: A potential high-level radioactive waste repository site

    Energy Technology Data Exchange (ETDEWEB)

    WoldeGabriel, G.; Broxton, D.E.; Bish, D.L.; Chipera, S.J. [Los Alamos National Lab., NM (United States)

    1992-12-31

    At Yucca Mountain, evidence for at least three distinct temporal groups of clinoptilolites can be delineated from the preliminary K/Ar dates (2 - 3 Ma; 4 - 5 Ma; 7 - 11 Ma). The older K/Ar dates that are similar to published illite/smectite ages (9-12 Ma) may be crystallization ages, whereas the younger dates probably represent continued diagenetic reactions of older clinoptilolites with percolating fluids. The K/Ar dates increase with depth, suggesting minimal argon loss in the deeper samples. internal consistency of the clinoptilolite K/Ar results at different levels within the drill holes suggest that dating of K-rich zeolites may provide useful information for assessing the zeolitization at Yucca Mountain. Variations in the K/Ar dates are probably related to Ar loss during dissolution of older clinoptilolites and to contamination by finely crystalline feldspars. 18 refs., 1 tab.

  16. Preliminary assessment of clinoptilolite K/Ar results from Yucca Mountain, Nevada: A potential high-level radioactive waste repository site

    Energy Technology Data Exchange (ETDEWEB)

    WoldeGabriel, G.; Bish, D.L.; Broxton, D.E.; Chipera, S.J.

    1992-03-01

    At Yucca Mountain, evidence for at least three distinct temporal groups of clinoptilolites can be delineated from the preliminary K/Ar dates (2--3 Ma; 4--5 Ma; 7--11 Ma). The older K/Ar dates that are similar to published illite/smectite ages (9--12 Ma) may be crystallization ages, whereas the younger dates probably represent continued diagenetic reactions of older clinoptilolites with percolating fluids. The K/Ar dates increase with depth, suggesting minimal argon loss in the deeper samples. Internal consistency of the clinoptilolite K/Ar results at different levels within the drill holes suggest that dating of K-rich zeolites may provide useful information for assessing the zeolitization at Yucca Mountain. Variations in the K/Ar dates are probably related to Ar loss during dissolution of older clinoptilolites and to contamination by finely crystalline feldspars.

  17. Southern Brasilia Belt (SE Brazil): tectonic discontinuities, K-Ar data and evolution during the Neoproterozoic Brasiliano orogeny

    Energy Technology Data Exchange (ETDEWEB)

    Valeriano, Claudio Morrison de [Universidade do Estado, Rio de Janeiro, RJ (Brazil)]. E-mail: cmval@uerj.br; Teixeira, Wilson [Sao Paulo Univ., SP (Brazil); Simoes, Luiz Sergio Amarante [UNESP, Sao Paulo, SP (Brazil); Heilbron, Monica [Conselho Nacional de Desenvolvimento Cientifico e Tecnologico (CNPq), Brasilia, DF (Brazil)

    2000-03-01

    This paper focuses the tectonic evolution of the southern brasilia belt, with emphasis on the Furnas segment, along the 21 deg C S parallel. The uppermost structural unit (Passos Nappe - PN) comprises a highly deformed metasedimentary succession interpreted as a fragment of the Neoproterozoic passive margin of western Sao francisco craton. An inverted metamorphic gradient ranging from greensvhits to lower granulite facies of medium to high-pressure regime characterizes the PN as relict of a subduction zone. The External Domain display a complex imbrication of basement rocks (Archean Piumhi greenstones, a turbiditic gaywacke succession and a calc-alkaline granitoid suite) with undated siliciclast low-grade metasedimentary rocks. The Sao Francisco Craton (SFC) comprises pre-1.8 Ga basement rocks covered by anchimetamorphic Neoproterozoic carbonatic shallow marine platform deposits of the Bambui group. The Brasiliano thrust stacking generated a coarse clastic influx of molassic character on the foreland zone of Sao Francisco Craton, coeval with the exhumation of the External Domain thrust sheets. New K-Ar determinations on mineral separates are presented an interpreted among previous data. The SFC basement rocks display Paleo-to Meesoproterozoic cooling ages. The allochthonous units, in contrast, display K-Ar ages within the 560-675 Ma range. Brasiliano thrust stacking is therefore interpreted to have taken place onto a cold Sao Francisco craton foreland, in a thin-skinned style, as basement rocks were not heated enough to have their-K-ar systems reset during the allochthony. (author)

  18. K-Ar age of young volcanic rocks and excess argon--Binary mixing model and quantitative study of excess argon effect

    Institute of Scientific and Technical Information of China (English)

    2000-01-01

    A binary mixing model for excess argon is suggested in the note. According to this model and the data of excess argon component obtained in our experiment , a quantitative study of the effect of excess argon on real K-Ar age of young volcanic rocks is done. The result indicates that the effect of 5% excess argon component in samples on K-Ar age of the samples more than 2 Ma is less than 7.36% and can lead K-Ar age of 0.5 Ma samples to increase by 32.4%, while 1% excess argon component leads K-Ar age of 0.5 Ma samples to increase by 6.26%. Therefore, when pre-processed excess argon component is ≤1%, K-Ar age of the samples more than 0.5 Ma should be credible. On this basis we suggest a principal opinion for evaluation of previous K-Ar dating results and propose that the matrix is used to determine K-Ar age of young volcanic rocks. For the samples less than 0.2 Ma, in the case of high excess argon content, even if only 1% excess argon component exists in their matrix, it can also greatly affect their K-A age. Thus it must be careful to treat the dating result.

  19. 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...

  20. K?Ar dating and geological significance of clastic sediments of the Paleocene Sepultura Formation, Baja California, México

    Science.gov (United States)

    Téllez Duarte, Miguel Agustín.; López Martínez, Margarita

    2002-12-01

    At its type locality, the Paleocene Sepultura Formation consists of two members: a lower glauconitic-rich clastic section and an upper calcareous section. Three samples of authigenic glauconite pellets from two localities with good clastic sediment exposures were dated using K-Ar. At the type locality of Mesa La Sepultura, pellets from the middle of the clastic section yield a date of 60±1 Ma (weighted average of four experiments), and pellets from the top of the clastic unit give a date of 60±1 Ma (weighted average of two experiments). Pellets from the base of the section at La Mesa, 60 km distant, give a date of 59±1 Ma (one experiment). Dates obtained are in good agreement with those reported by biostratigraphy and confirm a Late Danian age. Our results differ from those reported elsewhere, in which low potassium content glauconites yield younger K-Ar ages than expected. An explanation for our observed agreement in ages could be related to the tectonic setting of forearc basins, where the low geothermal gradient prevents argon loss and reliable dates can be obtained.

  1. 40Ar/39Ar and K/Ar dating of low grade metamorphism: examples on metabasites from Central Chile

    Science.gov (United States)

    Aguirre, L.; Feraud, G.; Fuentes, F.; Delbar, M.; Morata, D.

    2003-04-01

    Dating low to very low-grade burial metamorphic assemblages is often difficult because of (1) few mineral phases compositionally suitable to apply the 40Ar/39Ar and K-Ar methods, and (2) small amount in which these phases are commonly found. K-feldspar adularia, sericitic mica, and celadonite are the best known K-bearing secondary minerals. We present some successful attempts to analyse two distinct secondary phases from a same volcanic formation that allow to test the validity of the measured ages. These ages have been also compared with the crystallisation age of the volcanic rocks in which the secondary phases were lately developed. Adularia and sericite were selected from basic lava flows from a 3 to 13 km thick Cretaceous sequence from the Coastal Range of central Chile, at two different locations: the Bustamante Hill (west from Santiago), and the Cordón de Chacana, c. 80 km further north. Adularia came from a low-variance assemblage with pumpellyite, chlorite and low-albite contained in amygdules whereas sericite was present in milky-white strongly sericitized plagioclase crystals. While small clusters of rare fresh plagioclase grains from lava flows from Bustamante and Chacana displayed concordant plateau ages 119.4 ± 2.4 (2 sigma) and 118.7 ± 0.6 Ma, respectively, the adularia from the same formations gave sensibly younger ages around 94 Ma (high temperature steps), and 96.8 ± 0.2 Ma (plateau age) in Bustamante and Chacana, respectively. Sericite ages were measured in situ into single crystals of strongly transformed plagioclases. The relative proportion of sericite and plagioclase corresponding to each degasing step was monitored by measuring the Ca/K ratio (deduced from 37ArCa/39Ar_K). While intermediate ages were measured on some sericite of both sites (corresponding to a variable but permanent contribution of plagioclase on each step), a plateau age of 97.0 ± 1.6 Ma (concordant with adularia) could be obtained on a strongly sericitized plagioclase

  2. 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

  3. Charge-exchange, ionization and excitation in low-energy Li$^{+}-$ Ar, K$^{+}-$ Ar, and Na$^{+}-$He collisions

    CERN Document Server

    Lomsadze, Ramaz A; Kezerashvili, RomanYa; Schulz, Michael

    2016-01-01

    Absolute cross sections are measured for charge-exchange, ionization, and excitation within the same experimental setup for the Li$^{+}-$Ar, K$^{+}-$ Ar, and Na$^{+}-$ He collisions in the ion energy range $0.5-10$ keV. Results of our measurements along with existing experimental data and the schematic correlation diagrams are used to analyze and determine the mechanisms for these processes. The experimental results show that the charge-exchange processes are realized with high probabilities and electrons are predominately captured in ground states. The cross section ratio for charge exchange, ionization and excitation processes roughly attains the value $10:2:1$, respectively. The contributions of various partial inelastic channels to the total ionization cross sections are estimated and a primary mechanism for the process is defined. The energy-loss spectrum, in addition, is applied to estimate the relative contribution of different inelastic channels and to determine the mechanisms for the ionization and f...

  4. K-Ar Geochronology of Mesozoic Mafic Dikes in Shandong Province, Eastern China:Implications for Crustal Extension

    Institute of Scientific and Technical Information of China (English)

    LIU Shen; HU Ruizhong; ZHAO Junhong; FENG Caixia

    2004-01-01

    Based on K-Ar isotope analyses, Mesozoic mafic (and alkali ultramafic) dikes from western and eastern Shandong Province, China, are dated at 88.2±1.70 Ma to 169.5±3.7 Ma with the majority of ages ranging from 90 Ma to 140 Ma. The emplacement of the dikes suggests a major Yanshanian (Cretaceous) crustal extension in Shandong province.Together with other available age data, this study suggests four periods of crustal extension at about 80 Ma, 100 Ma, 120 Ma and 140 Ma, respectively. Besides the effect of collapse of the Yanshanian orogenic belt on the emplacement of the mafic dikes in Shandong in the Cretaceous, the mantle plume and the extensive left-lateral advection and extension of the Tanlu fault also have controlled the crustal extension and the emplacement of the mafic dikes in eastern Shandong and western Shandong, respectively.

  5. Noble Gas Analysis for Mars Robotic Missions: Evaluating K-Ar Age Dating for Mars Rock Analogs and Martian Shergottites

    Science.gov (United States)

    Park, J.; Ming, D. W.; Garrison, D. H.; Jones, J. H.; Bogard, D. D.; Nagao, K.

    2009-01-01

    The purpose of this noble gas investigation was to evaluate the possibility of measuring noble gases in martian rocks and air by future robotic missions such as the Mars Science Laboratory (MSL). The MSL mission has, as part of its payload, the Sample Analysis at Mars (SAM) instrument, which consists of a pyrolysis oven integrated with a GCMS. The MSL SAM instrument has the capability to measure noble gas compositions of martian rocks and atmosphere. Here we suggest the possibility of K-Ar age dating based on noble gas release of martian rocks by conducting laboratory simulation experiments on terrestrial basalts and martian meteorites. We provide requirements for the SAM instrument to obtain adequate noble gas abundances and compositions within the current SAM instrumental operating conditions, especially, a power limit that prevents heating the furnace above approx.1100 C. In addition, Martian meteorite analyses from NASA-JSC will be used as ground truth to evaluate the feasibility of robotic experiments to constrain the ages of martian surface rocks.

  6. K/Ar ages, magnetic stratigraphy and morphological evolution of La Gomera: implications for the Canary Islands hotspot evolution.

    Science.gov (United States)

    Paris, R.; Guillou, H.; Carracedo, J. C.; Pérez Torrado, F. J.

    2003-04-01

    The Canary Islands are a group of seven volcanic islands, 100-700 km west of the Sahara continental margin. The spatial and chronological evolution of the canarian volcanism, from east to west, is due to the progression of the slow-moving african plate on a hotspot. La Gomera is located between the western shield-growing stage islands (La Palma, 1,7 Ma and El Hierro, 1,1 Ma) and the central "rejuvaneted stage" islands (Tenerife, 11,9 Ma and Gran Canaria, 14,5 Ma). After 23 K-Ar ages and paleomagnetism datas, we determine the main volcanic phases of La Gomera : (1) the submarine shield volcano (> 9,5 Ma), (2) the first subaeriel shield volcano (9,43-7,36 Ma), (3) the Vallehermoso stratovolcan, (4) the peripheral "planèzes" and domes forming series (6,67-1,94 Ma) and the Garajonay horizontal series (5,42-4,25 Ma). The stratovolcano and the horizontal series fill a 10 km wide depression that is supposed to be a giant landslide embayment. The scarps of this landslide correspond to the main discontinuity in the island structure. After 4 M.y. of very scarce volcanism, the whole structure of La Gomera is in relief inversion, with a radial pattern of deep barrancos. The erosion rates are lower during the hiatus (< 0,2 m/ka) than during the shield stage (0,2-0,9 m/ka), pointing out the fact that the volcanic construction rates and the erosion rates are strongly correlated. La Gomera is one of the best example of a hiatus stage of hotspot evolution. The volcanic load La Gomera and Tenerife may have delayed the western islands volcanism, favouring a dual-line.

  7. Mineralogical, chemical and K-Ar isotopic changes in Kreyenhagen Shale whole rocks and pyrolysis experimental maturation

    Science.gov (United States)

    Clauer, Norbert; Lewan, Michael D.; Dolan, Michael P.; Chaudhuri, Sambhudas; Curtis, John B.

    2014-01-01

    Progressive maturation of the Eocene Kreyenhagen Shale from the San Joaquin Basin of California was studied by combining mineralogical and chemical analyses with K–Ar dating of whole rocks and pyrolysis of an immature outcrop sample. The K–Ar age decreases from 89.9 ± 3.9 and 72.4 ± 4.2 Ma for the outcrop whole rock and its <2 μm fraction, respectively, to 29.7 ± 1.5 and 21.0 ± 0.7 Ma for the equivalent materials buried to 5167 m. The natural maturation does not produce K–Ar ages in the historical sense, but rather K/Ar ratios of relative K and radiogenic 40Ar amounts resulting from a combined crystallization of authigenic and alteration of initial detrital K-bearing minerals of the rocks. The Al/K ratio of the naturally matured rocks is essentially constant for the entire depth sequence, indicating that there is no detectable variation in the crystallo-chemical organization of the K-bearing alumino-silicates with depth. No supply of K from outside of the rock volumes occurred, which indicates a closed-system behavior for it. Conversely, the content of the total organic carbon (TOC) content decreases significantly with burial, based on the progressive increasing Al/TOC ratio of the whole rocks. The initial varied mineralogy and chemistry of the rocks and their <2 μm fractions resulting from differences in detrital sources and depositional settings give scattered results that homogenize progressively during burial due to increased authigenesis, and concomitant increased alteration of the detrital material.

  8. The western Aeolian Islands volcanoes (South Tyrrhenian Sea): highlight on their eruptive history based on K-Ar dating.

    Science.gov (United States)

    Leocat, E.; Gillot, P.-Y.; Peccerillo, A.

    2012-04-01

    The Aeolian Islands volcanoes are located in southern Tyrrhenian Sea on the northern continental margin of the Calabro-Peloritan basement. The Stromboli, Panarea and Vulcano volcanoes of the half eastern sector are well studied as they are still active and they represent high volcanic hazard. While stratigraphic studies were carried out on volcanoes of the western sector, radiometric ages are lacking to well understand their eruptive history. Therefore, new geochronological and geochemical data were obtained for Alicudi, Filicudi, Salina and Lipari western volcanoes. The aim is to establish a complete time framework of the volcanism and to study possible time-related variations of magma compositions. The 37 new ages were obtained using K-Ar Cassignol-Gillot technique that is suitable for dating Quaternary volcanic rocks. The new geochemical data consist of whole rock major and trace elements analysis on dated samples. Our new sets of data give evidence that the Aeolian Islands are young volcanoes emplaced within the last 300 ka. The oldest products outcrop at Filicudi, Salina and Lipari. Te first emerged activity of Alicudi volcano occurred 120 ka ago. While quiescence activity of at least 50 ka is recognized at Filicudi and Lipari, and potentially at Salina, the volcanic activity of Alicudi would have been relatively continuous. These whole volcanoes were active within the last 30 ka which has to be considered for volcanic hazard assessment. At the scale of each volcano, the degree of differentiation increase roughly through time, except at Filicudi where the ultimate products correspond to mafic magma. At the scale of the archipelago, this process increases from western Alicudi and Filicudi volcanoes, where andesitic magmas are the most evolved magmas, to central Salina and Lipari volcanoes, where rhyolitic magmas are emitted during explosive eruption. Moreover, pulses of magmatic activity would have occurred around 30-40 and 110-120 ka when the four volcanoes

  9. O granito de Coentral revisitado: idade U-Pb de zircão

    OpenAIRE

    Gomes, E. M. C.; Antunes, I. M.H.R.

    2011-01-01

    O granito de Coentral forma um pequeno plutonito, aflorante no bordo oeste da Zona Centro Ibérica, próximo do limite com a Zona de Ossa Morena, que intruiu metassedimentos do Grupo das Beiras. Trabalhos anteriores de datação radiométrica K-Ar de moscovites e biotites sugeriram a sua implantação no Neoproterozóico superior a Câmbrico inferior e posterior deformação e metamorfismo hercínicos. Novos dados isotópicos U-Pb ID-TIMS de zircão indicam uma idade de implantação para o granito de Co...

  10. Clay mineral provinces in tidal mud flats at Germany's North Sea coast with illite K-Ar ages potentially modified by biodegradation

    Science.gov (United States)

    Brockamp, Olaf; Clauer, Norbert

    2012-07-01

    Mineralogical studies, chemical analyses and K-Ar dating were carried out on clay fractions from tidal mud flats along the Lower Saxony coast and its bays to identify material sources and sedimentary processes at this dynamic interface between air, land and sea. From the coast into the bays, sediments are enriched in fine-grained smectite relative to the coarser grained illite, chlorite and kaolinite, due to the weakening of the tidal current energy in the bays. In addition, the study area can be divided into two provinces on the basis of the illite K/Rb ratios and Mg contents. To the west [Schiermonnikoog, Dollart, Ley Bay up to Norderney island], longshore currents carry suspensions from the Belgian and Dutch coasts; to the east [from Langeoog island, Jade Bay to the Helgoland mud area] suspensions from the Elbe and Weser rivers are mixed with submarine reworked glacial sediments, whereas the portion of longshore current suspensions from the west decreases, becoming negligible in the Helgoland mud area off the Elbe and Weser estuaries. The illite K-Ar data vary considerably and fail as source indicators due to differential settling and mixing of the clay material and probably to Ar loss from illite by biodegradation during digestive processes. Only further offshore, outside the zone of dynamic sediment dispersion, do the K-Ar data fit provenance patterns.

  11. O Poder Régio ou Estado?! Debate Historiográfico e apontamentos para uma nova conceitualização da gestão do Poder na Idade Média * The Royal Power or State?! Historiographical Debate and notes towards a new conceptualization of the exercise of Power...

    Directory of Open Access Journals (Sweden)

    THIAGO PEREIRA DA SILVA MAGELA

    2014-02-01

    Full Text Available Resumo: Buscamos traçar um panorama do debate acerca da validade do conceito de Estado para o Ocidente medieval, bem como buscamos avançar um modelo explicativo para entendermos o Estado na Idade Média castelhana. Além disso, traçamos em linhas gerais, a constituição do Estado Castelhano até o reinado de Afonso X. O artigo finaliza propondo uma dupla fratura com as visões de que a Idade Média não teve Estados, bem como aquela que advoga em nome de um precoce Estado Moderno. O Estado Feudal castelhano está dentro da lógica de articulação da Sociedade Feudal.Palavras-chave: Estado Feudal – Castela – Política. Abstract: We intend to delineate an overview of the debate regarding the validity of the concept of State to the medieval West, and, in like manner,we also seek to advance an explanatory model for understanding the rising of the State in Castillan Middle Ages. Besides that, we also traced , in a quite general way, the formation of the Castillan state until the reign of Alfonso X. The article concludes proposing a double rupture with the lines of thought that affirm  a non-States Middle Ages ,  likewise the one that defends a precocious Modern State. The Castillan Feudal State is located within the logic of articulation of Feudal Society.Keywords: Feudal State – Castile – Politics.

  12. An in-situ K-Ar isochron dating method for planetary landers using a spot-by-spot laser-ablation technique

    Science.gov (United States)

    Cho, Yuichiro; Sugita, Seiji; Miura, Yayoi N.; Okazaki, Ryuji; Iwata, Naoyoshi; Morota, Tomokatsu; Kameda, Shingo

    2016-09-01

    Age is essential information for interpreting the geologic record on planetary surfaces. Although crater counting has been widely used to estimate the planetary surface ages, crater chronology in the inner solar system is largely built on radiometric age data from limited sites on the Moon. This has resulted in major uncertainty in planetary chronology. Because opportunities for sample-return missions are limited, in-situ geochronology measurements from one-way lander/rover missions are extremely valuable. Here we developed an in-situ isochron-based dating method using the K-Ar system, with K and Ar in a single rock sample extracted locally by laser ablation and measured using laser-induced breakdown spectroscopy (LIBS) and a quadrupole mass spectrometer (QMS), respectively. We built an experimental system combining flight-equivalent instruments and measured K-Ar ages for mineral samples with known ages (~1.8 Ga) and K contents (1-8 wt%); we achieved precision of 20% except for a mineral with low mechanical strength. Furthermore, validation measurements with two natural rocks (gneiss slabs) obtained K-Ar isochron ages and initial 40Ar consistent with known values for both cases. This result supports that our LIBS-MS approach can derive both isochron ages and contributions of non-in situ radiogenic 40Ar from natural rocks. Error assessments suggest that the absolute ages of key geologic events including the Noachian/Hesperian- and the Hesperian/Amazonian-transition can be dated with 10-20% errors for a rock containing ~1 wt% K2O, greatly reducing the uncertainty of current crater chronology models on Mars.

  13. Edades K/Ar de 54 rocas ígneas y metamórficas del occidente, centro y sur de México

    OpenAIRE

    Jesús Solé; Juan Carlos Salinas; Enrique González Torres; José Eduardo Cendejas Cruz

    2007-01-01

    Se presenta un listado y se discuten las edades K/Ar de 54 muestras de rocas ígneas y metamórficas de varias localidades de México determinadas en el marco de un convenio entre el Consejo de Recursos Minerales (ahora Servicio Geológico Mexicano) y el Instituto de Geología de la Universidad Nacional Autónoma de México. Se analizaron rocas de los siguientes estados: Baja California Sur, Colima, Durango, Estado de México, Guerrero, Jalisco, Oaxaca, San Luis Potosí, Sinaloa y Zacatecas. Se report...

  14. White mica K-Ar geochronology of HP-UHP units in the Lago di Cignana area, western Alps, Italy: Tectonic implications for exhumation

    Science.gov (United States)

    Gouzu, Chitaro; Yagi, Koshi; Thanh, Ngo Xuan; Itaya, Tetsumaru; Compagnoni, Roberto

    2016-04-01

    High-pressure and ultra-high pressure (HP-UHP) blueschist- and eclogite-facies metabasaltic and metasedimentary rocks occur in four different tectonic units near Lago di Cignana, western Alps. We have determined K-Ar ages for white micas (matrix phengite and paragonite) from the Lago di Cignana UHP unit (LCU; 39-41 Ma); the lower and upper units of the Zermatt-Saas meta-ophiolite (LU and UU; 37-38 Ma and 38-41 Ma respectively), and the Combin unit (CU; 36-40 Ma). These K-Ar ages overlap with single-grain Ar-Ar plateau ages (36-42 Ma) previously determined for phengites from LCU metasediments. Matrix white micas have been severely deformed during exhumation, and their chemistries differ from those of micas included in garnet. Although individual mica grains in the matrix could have experienced different degrees of deformation which have reset their K-Ar systems, "bulk" white mica separates provide the average age of all the individual grains in the separate. The similarity of ages determined for white micas from the LCU, LU, UU and CU units, regardless of rock type and mineral species, suggests that these four units were metamorphosed together as part of a single metamorphic sequence in the Piemonte-Liguria paleosubduction zone and were subsequently exhumed together. However, present-day structural relationship among those units and the limited occurrence of UHP minerals in LCU suggests that the exhumation of LCU was more rapid than that for LU, UU and CU. The age gaps between the youngest value of white mica K-Ar ages in each unit and the inferred timing of the metamorphic peak (U-Pb age: 44 Ma) is 5, 7, 6 and 8 Myr for LCU, LU, UU and CU, respectively. These intervals are considerably shorter than that determined for the Sanbagawa HP metamorphic belt of Southwest Japan (> 31 Myr). The short interval observed for the Lago di Cignana units that we have studied is consistent with the model of rapid exhumation of the UHP-bearing metamorphic domain, suggesting the

  15. 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.

  16. Dataciones radiometricas (14C y K/Ar del Teide y el Rift noroeste, Tenerife, Islas Canarias

    Directory of Open Access Journals (Sweden)

    Hansen, A.

    2003-08-01

    unstable slopes of Teide, it took place without any apparent response of the volcano; on the contrary, these eruptions seemed to progressively buttress and enhance the stability of Teide Volcano. Conversely, the occurrence of these flank eruptions, combined with the Pico Viejo and NW rift eruptions, poses a very high lava-flow risk to the now densely populated areas in north and west Tenerife, which have been almost entirely resurfaced during the past 20,000 years.El Teide, el edificio volcánico más alto del planeta (3.718 m sobre el nivel del mar, > 7 km desde el fondo oceánico después del Mauna Loa y Mauna Kea en las islas Hawaii, forma un complejo volcánico en el centro de la isla de Tenerife. Su actividad eruptiva reciente (últimos 20 Ka está asociada con la rama NO del rift triple (120" que ha configurado la etapa reciente de construcción de la isla. La mayoría de las erupciones de Tenerife en este período se han localizado en estas estructuras volcánicas, generando frecuentes y extensas coladas máficas y félsicas, muchas alcanzado la costa e invadiendo lo que es ahora una de las zonas más densamente pobladas de Tenerife y, probablemente, de cualquier isla oceánica del planeta. Sin embargo, y a pesar de los numerosos estudios y proyectos previos, falta aún información geológica básica para este importante sistema volcánico, en particular la datación de las diferentes erupciones que lo componen, con objeto de reconstruir el marco geocronológico indispensable para conocer su evolución y determinar científicamente los riesgos volcánicos, de perentoria necesidad habida cuenta de su naturaleza y entidad, y de la población potencialmente afectada. Nuevas dataciones de Carbono-14 y K/Ar aportan ahora importante información a este respecto. La mayoría de las erupciones de los últimos 20 Ka no están relacionadas con el estratovolcán Teide, que sólo ha tenido una hace 1.240 f 60 años -entre 663 y 943 AD una vez calibrada la edad-, sino con el

  17. Nuclear geochronology. Chapter 6: Sedimentary rocks dating by the Rubidium-Strontium (Rb/Sr) and Potassium-Argon (K/Ar) radiometric methods; Geocronologia nuclear. Capitulo 6: Datacao de rochas sedimentares pelos metodos radiometricos rubidio-estroncio (Rb/Sr) e potassio-argonio (K/Ar)

    Energy Technology Data Exchange (ETDEWEB)

    Thomaz Filho, Antonio [Universidade do Estado, Rio de Janeiro, RJ (Brazil). Inst. de Geociencias; Mizusaki, Ana Maria Pimentel [Rio Grande do Sul Univ., Porto Alegre, RS (Brazil). Inst. de Geociencias; Kawashita, Koji [Sao Paulo Univ., SP (Brazil). Inst. de Geociencias; Torquato, Joaquim Raul [Ceara Univ., Fortaleza, CE (Brazil). Dept. de Geologia

    1995-12-31

    The paper deals with the Rubidium/Strontium (Rb/Sr) and Potassium/Argon (K/Ar) radiometric methods application in the sedimentary rocks dating, including the methodology, the method restrictions and the ages meaning. The work concludes that the sedimentary rocks radiometric dating, by the Rb/Sr method is possible, furnishing results geologically significant. The {sup 87} Sr/{sup 86} Sr of marine carbonates has propitiated, mainly in the last years, the dating possibility of sedimentary rocks. The K/Ar radiometric method has been applied to determine the diagenetic events age of the sedimentary rocks, including its application in mesozoic and recent rocks, where the RB/Sr radiometric method presents some limitations 71 refs., 18 figs.

  18. Mineralogy and clinoptilolite K/Ar results from Yucca Mountain, Nevada, USA: A potential high-level radioactive waste repository site

    Energy Technology Data Exchange (ETDEWEB)

    WoldeGabriel, G.; Broxton, D.E.; Bish, D.L.; Chipera, S.J.

    1993-11-01

    The Yucca Mountain Site Characterization Project is investigating Yucca Mountain, Nevada, as a potential site for a high-level nuclear waste repository. An important aspect of this evaluation is to understand the geologic history of the site including the diagenetic processes that are largely responsible for the present-day chemical and physical properties of the altered tuffs. This study evaluates the use of K/Ar geochronology in determining the alteration history of the zeolitized portions of Miocene tuffs at Yucca Mountain. Clinoptilolite is not generally regarded as suitable for dating because of its open structure and large ion-exchange capacity. However, it is the most abundant zeolite at Yucca Mountain and was selected for this study to assess the feasibility of dating the zeolitization process and/or subsequent processes that may have affected the zeolites. In this study we examine the ability of this mineral to retain all or part of its K and radiogenic Ar during diagenesis and evaluate the usefulness of the clinoptilolite K/Ar dates for determining the history of alteration.

  19. Feasibility study of the immunogenicity and safety of a novel DTPw/Hib (PRP-T Brazilian combination compared to a licensed vaccine in healthy children at 2, 4, and 6 months of age Estudo de viabilidade de imunogenicidade e segurança de uma nova vacina brasileira combinada DTPw/Hib (PRP-T, comparada com uma vacina registrada, em crianças de 2, 4 e 6 meses de idade

    Directory of Open Access Journals (Sweden)

    SueAnn Costa Clemens

    2003-06-01

    Full Text Available Vaccination of infants with conjugated Haemophilus influenzae type b (Hib vaccines has been proven to reduce Hib meningitis by 95% and pneumoniae by 20%. The routine use of Hib vaccine is facilitated by the introduction of combination vaccines into the EPI (Expanded Plan of Immunization. The objective of this study was to compare the immunogenicity and reactogenicity of an extemporaneously mixed DTPw/Hib (diphtheria-tetanus-whole cell pertussis combination, using the technology of two Brazilian manufacturers, against a licensed DTPw/Hib European combination in 108 infants vaccinated at 2, 4 and 6 months according to the local national schedule. The Brazilian combination was highly immunogenic with Hib seroprotection rates (anti-PRP > 0.15 mg /ml of 98% after 2 doses and 100% after 3. Also for tetanus and pertussis the new Brazilian combination was as immunogenic as the European counterpart, except the diphtheria seroprotection rates and titers were lower. There was also no clinically relevant difference in reactogenicity. If these feasibility results are confirmed, the Brazilian DTPw/Hib combination should help to boost the uptake of Hib vaccination in Brazil.A vacinação contra (Haemophilus influenzae tipo b (Hib, utilizando vacinas conjugadas, provou reduzir em 95% os casos de meningite e em 20% as pneumonias por Hib. O uso rotineiro da vacina Hib foi facilitado pela introdução das vacinas combinadas no Programa Ampliado de Imunização (PAI. O objetivo deste estudo foi comparar a imunogenicidade e reatogenicidade da mistura extemporânea da vacina combinada contra difteria-tétano-pertussis de células inteiras/Haemophilus influenzae (DTPw/Hib, de tecnologia e produção de 2 fabricantes brasileiros, à vacina européia registrada DTPw/Hib. Estudo realizado em 108 crianças em idade de 2, 4 e 6 meses, seguindo o esquema nacional de imunização. A vacina combinada brasileira foi altamente imunogênica, apresentando taxas de soroprote

  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. Quantitative Potassium Measurements with Laser-Induced Breakdown Spectroscopy Using Low-Energy Lasers: Application to In Situ K-Ar Geochronology for Planetary Exploration.

    Science.gov (United States)

    Cho, Yuichiro; Horiuchi, Misa; Shibasaki, Kazuo; Kameda, Shingo; Sugita, Seiji

    2017-08-01

    In situ radiogenic isotope measurements to obtain the absolute age of geologic events on planets are of great scientific value. In particular, K-Ar isochrons are useful because of their relatively high technical readiness and high accuracy. Because this isochron method involves spot-by-spot K measurements using laser-induced breakdown spectroscopy (LIBS) and simultaneous Ar measurements with mass spectrometry, LIBS measurements are conducted under a high vacuum condition in which emission intensity decreases significantly. Furthermore, using a laser power used in previous planetary missions is preferable to examine the technical feasibility of this approach. However, there have been few LIBS measurements for K under such conditions. In this study, we measured K contents in rock samples using 30 mJ and 15 mJ energy lasers under a vacuum condition (10(-3 )Pa) to assess the feasibility of in situ K-Ar dating with lasers comparable to those used in NASA's Curiosity and Mars 2020 missions. We obtained various calibration curves for K using internal normalization with the oxygen line at 777 nm and continuum emission from the laser-induced plasma. Experimental results indicate that when K2O laser energy, with a detection limit of 88 ppm and 20% of error at 2400 ppm of K2O. Futhermore, the calibration curve based on the K 769 nm line intensity normalized with continuum emission yielded the best result for the 15 mJ laser, giving a detection limit of 140 ppm and 20% error at 3400 ppm K2O. Error assessments using obtained calibration models indicate that a 4 Ga rock with 3000 ppm K2O would be measured with 8% (30 mJ) and 10% (15 mJ) of precision in age when combined with mass spectrometry of (40)Ar with 10% of uncertainty. These results strongly suggest that high precision in situ isochron K-Ar dating is feasible with a laser used in previous and upcoming Mars rover missions.

  2. Rb, Sr and strontium isotopic composition, K/Ar age and large ion lithophile trace element abundances in rocks and glasses from the Wanapitei Lake impact structure

    Science.gov (United States)

    Winzer, S. R.; Lum, R. K. L.; Schuhmann, S.

    1976-01-01

    Shock metamorphosed rocks and shock-produced melt glasses from the Wanapitei Lake impact structure have been examined petrographically and by electron microprobe. Eleven clasts exhibiting varying degrees of shock metamorphism and eight impact-produced glasses have been analyzed for Rb, Sr and Sr isotopic composition. Five clasts and one glass have also been analyzed for large ion lithophile (LIL) trace element abundances including Li, Rb, Sr, and Ba and the REE's. The impact event forming the Wanapitei Lake structure occurred 37 m.y. ago based on K/Ar dating of glass and glassy whole-rock samples. Rb/Sr isotopic dating failed to provide a meaningful whole-rock or internal isochron. The isotopic composition of the glasses can be explained by impact-produced mixing and melting of metasediments.

  3. Sm-Nd, K-Ar and petrologic study of some kimberlites from eastern United States and their implication for mantle evolution

    Science.gov (United States)

    Basu, A.R.; Rubury, E.; Mehnert, H.; Tatsumoto, M.

    1984-01-01

    We provide new data on Sm-Nd systematics, K-Ar dating and the major element chemistry of kimberlites from the eastern United States (mostly from central New York State) and their constituent mineral phases of olivine, clinopyroxene, garnet, phlogopite and perovskite. In addition, we report Nd-isotopes in a few kimberlites from South Africa, Lesotho and from the eastern part of China. The major element compositions of the New York dike rocks and of their constituent minerals including a xenolith of eclogite are comparable with those from the Kimberley area in South Africa. The K-Ar age of emplacement of the New York dikes is further established to be 143 Ma. We have analyzed the Nd-isotopic composition of the following kimberlites and related rocks: Nine kimberlite pipes from South Africa and Lesotho, two from southern India; one from the U.S.S.R., fifteen kimberlite pipes and related dike rocks from eastern and central U.S. and two pipes from the Shandong Province of eastern China. The age of emplacement of these kimberlites ranges from 1300 million years to 90 million years. The initial Nd-isotopic compositions of these kimberlitic rocks expressed as e{open}NdIwith respect to a chondritic bulk-earth growth-curve show a range between 0 and +4, with the majority of the kimberlites being in the range 0 to +2. This range is not matched by any other suite of mantle-derived igneous rocks. This result strengthens our earlier conclusion that kimberlitic liquids are derived from a relatively primeval and unique mantle reservoir with a nearly chondritic Sm/Nd ratio. ?? 1984 Springer-Verlag.

  4. Structural evolution of the Yeongwol thrust system, northeastern Okcheon fold-thrust belt, Korea: Insights from structural interpretations and SHRIMP U-Pb and K-Ar geochronology

    Science.gov (United States)

    Jang, Yirang; Kwon, Sanghoon

    2017-04-01

    The NE-trending Okcheon Belt is a prominent fold-thrust belt preserved in the Korean Peninsula. In the Yeongwol area, the northeastern Okcheon Belt, the Cambrian-Ordovician (possibly to Silurian) Joseon Supergroup overlies the Carboniferous-Permian (possibly to early Triassic) Pyeongan Supergroup and/or Jurassic Bansong Group by N-S trending thrust faults, having highly connected traces in map view. To understand the structural geometry of these thrust faults and their evolution history, we have conducted structural analyses, together with SHRIMP U-Pb zircon and K-Ar illite age datings. The results show that (1) the thrusts in the Yeongwol area, carrying the lower Paleozoic strata over the upper Paleozoic or Mesozoic strata, are defined as the Yeongwol thrust system. The closed-loops map patterns of this system can further be interpreted by alternative duplex models in terms of a hinterland dipping duplex vs. a combination of major thrusts and connecting splays; (2) newly obtained SHRIMP U-Pb zircon ages from a dike and synorogenic sediments and K-Ar illite ages from fault gouges, together with previously reported evidences form the Yeongwol area, suggest multiple events after Permo-Triassic to early Neogene. The SHRIMP U-Pb detrital zircon ages from the lower Paleozoic rocks of the Yeongwol area can provide tectono-stratigraphic information of this area before the Permian. These further indicate the broader implications in that how detailed structural interpretations supported by the geochronological data can help to understand the tectonic evolution of the Okcheon Belt as well as the fold-thrust belts in general.

  5. Comparative 40Ar/39Ar and K-Ar dating of illite-type clay minerals: A tentative explanation for age identities and differences

    Science.gov (United States)

    Clauer, Norbert; Zwingmann, Horst; Liewig, Nicole; Wendling, Raymond

    2012-10-01

    The 40K/40Ar (K-Ar) and 40Ar/39Ar dating methods are applied here to the same, very small, micrometric illite-type particles that crystallized under low-temperature (samples with a total of fifteen size fractions from advantages, such as the plateaus obtained by incremental step heating of the various size fractions, even if not translatable straight as ages of the illite populations; they allow identification of two generations of authigenic illite that formed at about 200 and 175 Ma, and one detrital generation. However, 40Ar/39Ar dating of clay minerals remains challenging as technical factors, such as the non-standardized encapsulation, may have potential unexpected effects. Both dating methods have their limitations: (1) K-Ar dating requires relatively large samples (ca. 10-20 mg) incurring potential sample homogeneity problems, with two aliquots required for K and Ar analysis for an age determination, also inducing a higher analytical uncertainty; (2) an identified drawback of 40Ar/39Ar dating is Ar recoil and therefore potential loss that occurs during neutronic creation of 39Ar from 39K, mostly in the finer mineral particles. If all the recoiled 39Ar is redistributed into adjacent grains/minerals, the final 40Ar/39Ar age of the analyzed size fraction remains theoretically identical, but it is not systematic in clay-type material. The finest grain sizes (e.g., convenient and straightforward use supported by a standardized and well-controlled technical approach. The present comparison of the two Ar-dating methods as applied to clay material shows that neither method is presently outdated, and that they are even of reciprocal use. Both methods have distinct application fields in clay geochronology and complementary application fields in clay crystallography.

  6. Episodes of brittle deformation within the Dien Bien Phu Fault zone, Vietnam: Evidence from K-Ar age dating of authigenic illite

    Science.gov (United States)

    Bui, Hoang Bac; Ngo, Xuan Thanh; Khuong, The Hung; Golonka, Jan; Nguyen, Tien Dung; Song, Yungoo; Itaya, Tetsumaru; Yagi, Koshi

    2017-01-01

    Constraining the timing of fault zone origin and movement history is of fundamental geotectonic importance to understand the evolution and processes of the brittle fault structures. The authors present in this paper authigenic illite K-Ar age data from the fault gouge samples, collected from the Dien Bien Phu Fault (DBPF) in the Dien Bien province, Vietnam as well as in a major strike-slip fault zone in South-East Asia; all of which played important roles in the structural formation and geotectonic development of northwestern Vietnam. The gouge fault samples were separated into four grain-size fractions (groups, from 26 to 29 Ma and 130 Ma. The timing of the fault movements is defined at 26 ± 0.24 Ma, 29 ± 0.61 Ma, 130.1 ± 1.27 Ma and 130.7 ± 1.29 Ma. This indicates that the Dien Bien Phu Fault underwent two movements, first in the Early Cretaceous, with an age of about 130 Ma and second in the Oligocene (Paleogene), with an age of about 26-29 Ma. The ductile deformation of the DBPF terminated during the Early Cretaceous. These studies also indicate slow exhumation of the Dien Bien granitoid complex during the Cretaceous times. The Oligocene ages indicate that the DBPF had been reactivated by the SE extrusion and clock-wise rotation of the Indochina block, caused by the collision of the Indian and Eurasian plates. This tectonic event led to the DBPF brittle-sinistral movement, causing the exhumation phase along the fault. This movement period (ca. 26-29 Ma) is coexistent with 600-700 km sinistral shearing along the Red River-Ailao Shan fault. This is the first report determining the absolute age constraints of multi-activated tectonic events, affecting the Dien Bien Phu Fault using the K-Ar dating method for the gouge samples.

  7. 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.

  8. Idade dos ratos versus idade humana: qual é a relação?

    OpenAIRE

    Andreollo, Nelson Adami; Elisvânia Freitas dos SANTOS; Araújo,Marina Rachel; Luiz Roberto LOPES

    2012-01-01

    RACIONAL: Milhões de ratos são empregados anualmente em pesquisas e no ensino. A exata relação entre a idade dos ratos, comparada com a idade dos humanos ainda é assunto de discussão e controvérsias. OBJETIVO: É revisar a literatura, analisando a idade dos ratos em comparação com a idade dos homens. MÉTODOS: Foram revisadas as publicações existentes sobre o assunto contidas nas bases Medline/Pubmed, Scielo, Biblioteca Cochrane e Lilacs cruzando os descritores ratos, cirurgia experimental e fi...

  9. 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...

  10. Avaliação da qualidade da casca dos ovos provenientes de matrizes pesadas com diferentes idades

    Directory of Open Access Journals (Sweden)

    V.M. Barbosa

    2012-08-01

    Full Text Available Foi realizado um estudo sobre qualidade da casca dos ovos incubáveis provenientes de matrizes pesadas com diferentes idades, por meio da avaliação da relação entre peso da casca e peso do ovo e análises de peso específico, espessura, porosidade, resistência e microscopia eletrônica. Os dois tratamentos foram definidos pela idade da matriz, sendo considerados ovos de matrizes novas - 33 semanas - e de matrizes velhas - 63 semanas. Os ovos de matrizes com 33 semanas foram mais leves, e o número de poros por cm² foi menor que o de ovos das aves mais velhas. Ovos de aves com 63 semanas apresentaram menor percentual de casca em relação ao peso do ovo, menor peso específico e menores resistência e espessura da casca. A proporção das membranas da casca em relação à sua espessura total foi maior nas matrizes mais novas. Concluiu-se que ovos de matrizes velhas têm qualidade de casca inferior aos ovos das matrizes novas e que as membranas da casca nos ovos de matrizes novas desempenham papel relevante em sua estrutura.

  11. K-Ar age and geochemistry of the SW Japan Paleogene cauldron cluster: Implications for Eocene-Oligocene thermo-tectonic reactivation

    Science.gov (United States)

    Imaoka, T.; Kiminami, K.; Nishida, K.; Takemoto, M.; Ikawa, T.; Itaya, T.; Kagami, H.; Iizumi, S.

    2011-01-01

    Systematic K-Ar dating and geochemical analyses of Paleogene cauldrons in the Sanin Belt of SW Japan have been made to explore the relationship between the timing of their formation and the Paleogene subduction history of SW Japan documented in the Shimanto accretionary complex. We also examine the magma sources and tectonics beneath the backarc region of SW Japan at the eastern plate boundary of Eurasia. Fifty-eight new K-Ar ages and 19 previously reported radiometric age data show that the cauldrons formed during Middle Eocene to Early Oligocene time (43-30 Ma), following a period of magmatic hiatus from 52 to 43 Ma. The hiatus coincides with absence of an accretionary prism in the Shimanto Belt. Resumption of the magmatism that formed the cauldron cluster in the backarc was concurrent with voluminous influx of terrigenous detritus to the trench, as a common tectono-thermal event within a subduction system. The cauldrons are composed of medium-K calc-alkaline basalts to rhyolites and their plutonic equivalents. These rocks are characterized by lower concentrations of large ion lithophile elements (LILE) including K 2O, Ba, Rb, Th, U and Li, lower (La/Yb) n ratios, lower initial Sr isotopic ratios (0.7037-0.7052) and higher ɛNd( T) values (-0.5 to +3.5) relative to Late Cretaceous to Early Paleogene equivalents. There are clear trends from enriched to depleted signatures with decreasing age, from the Late Cretaceous to the Paleogene. The same isotopic shift is also confirmed in lower crust-derived xenoliths, and is interpreted as mobilization of pre-existing enriched lithospheric mantle by upwelling depleted asthenosphere. Relatively elevated geothermal gradients are presumed to have prevailed over wide areas of the backarc and forearc of the SW Japan arc-trench system during the Eocene to Oligocene. Newly identified Late Eocene low silica adakites and high-Mg andesites in the Sanin Belt and Early Eocene A-type granites in the SW Korea Peninsula probably formed

  12. Chemical, petrographic, and K-Ar age data to accompany reconnaissance geologic strip map from Kingman to south of Bill Williams Mountain, Arizona

    Energy Technology Data Exchange (ETDEWEB)

    Arney, B.; Goff, F.; Eddy, A.C.

    1985-04-01

    As part of a reconnaissance mapping project, 40 chemical analyses and 13 potassium-argon age dates were obtained for Tertiary volcanic and Precambrian granitic rocks between Kingman and Bill Williams Mountain, Arizona. The dated volcanic rocks range in age from 5.5 +- 0.2 Myr for basalt in the East Juniper Mountains to about 25 Myr for a biotite-pyroxene andesite. The date for Picacho Butte, a rhyodacite in the Mt. Floyd volcanic field, was 9.8 +- 0.07 Myr, making it the oldest rhyodacite dome in that volcanic field. Dated rocks in the Fort Rock area range from 20.7 to 24.3 Myr. No ages were obtained on the Precambrian rocks. Compositionally, the volcanic rocks analyzed range from alkali basalt to rhyolite, but many rocks on the western side of the map area are unusually potassic. The granites chosen for analysis include syenogranite from the Hualapai Mountains, a muscovite granite from the Picacho Butte area, and two other granites. The chemical and K-Ar age data and petrographic descriptions included in this report accompany the reconnaissance geologic strip map published as LA-9202-MAP by Goff, Eddy, and Arney. 9 refs., 4 figs., 2 tabs.

  13. 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!

  14. 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.

  15. Novas configurações das eleições na idade mídia

    Directory of Open Access Journals (Sweden)

    Antonio Albino Canelas Rubim

    2001-11-01

    Full Text Available No mundo contemporâneo, o surgimento e desenvolvimento da comunicação midiática, e a conformação de uma sociabilidade estruturada e ambientada pela mídia recolocam em intensa evidência a temática do relacionamento entre política e comunicação. A interação entre mídia e eleições é tomada aqui como emblemática das transformações.In the contemporary world, the emergence and the development of a mediatic communication, and the conformation of a sociability structured by the media put in evidence the relationship between politics and communication. The interaction between media and elections is analyzed in this article as the emblematic example of these transformations.

  16. Novas configurações das eleições na idade mídia

    OpenAIRE

    Antonio Albino Canelas Rubim

    2001-01-01

    No mundo contemporâneo, o surgimento e desenvolvimento da comunicação midiática, e a conformação de uma sociabilidade estruturada e ambientada pela mídia recolocam em intensa evidência a temática do relacionamento entre política e comunicação. A interação entre mídia e eleições é tomada aqui como emblemática das transformações.In the contemporary world, the emergence and the development of a mediatic communication, and the conformation of a sociability structured by the media put in evidence ...

  17. Petrología y edad K/Ar de diques relacionados a la Formación Oncán, sierra de Ambargasta, Santiago del Estero Petrology and K/Ar age of dikes related to Oncán Formation, Santiago del Estero

    Directory of Open Access Journals (Sweden)

    MJ Correa

    2003-12-01

    Full Text Available Al noroeste de la sierra de Ambargasta, Santiago del Estero, en las cercanías de los puestos El Remanso y El Simbolar, aflora un enjambre de diques longitudinales de orientación predominante nordeste-sudoeste. La edad obtenida de 483±14 Ma (K/Ar roca total permite considerar a esta unidad como representativa de la culminación del magmatismo originado durante la aproximación y posterior colisión del terreno Pampia con el cratón del Río de La Plata. La presente contribución contiene además datos geoquímicos y petrográficos de esta litología, cuyas características permitieron correlacionarlos con el Pórfido Riodacítico Oncán. Poseen una composición granítica levemente peraluminosa y características geoquímicas similares a los granitoides más evolucionados de la sierra de Ambargasta.At the northwest of Ambargasta range, Santiago del Estero, near El Remanso and El Simbolar villages, a swarm of longitudinal dikes with a predominant NE trend crops out. The obtained age of 483±14 Ma (K/Ar WR, allows to consider this unit representative of the end of the magmatism originated during the approximation and subsequent collision of the Pampia terrane with the Río de La Plata craton. Geochemical and petrographic data allowed to correlate these rocks with the Oncán Rhyodacitic Porphyry. The studied rocks have a granitic composition, lightly peraluminous and geochemical characteristics similar to the highly evolved granitoids from the Sierra de Ambargasta.

  18. K/Ar chronologies of tephra units from the Middle Jurassic Sundance, and Late Early Cretaceous Mowry and Shell Creek Formations, Big Horn Basin, WY

    Science.gov (United States)

    Jiang, H.; Meyer, E. E.; Johnson, G. D.

    2013-12-01

    The Middle Jurassic Sundance and Late Early Cretaceous Shell Creek and Mowry Formations of the Big Horn Basin, Wyoming, contain an extensive record of altered tephra. These tephra are likely related to contemporary volcanic activity in the Sierra Nevada and various Coast Range terranes to the west and provide valuable chronometric control on the sedimentary record within a portion of the Sevier-aged and later Cordilleran foreland basin. In addition, several of these altered tephra (bentonites) provide a valuable economic resource. Despite the prominence of these strata across the basin, few isotopic ages have been reported to date. Here we present new K/Ar ages on biotite phenocrysts from those tephra occurrences as a chronometric check on samples that contained zircons with significant Pb loss, that preclude more precise U/Pb age determinations. A bulk biotite sample extracted from an altered tuff in the Lower Sundance Formation gives an age of 167.5 × 5 Ma. This tuff occurs just above a dinosaur track-bearing peritidal sequence. Bulk biotite ages from the lower Shell Creek Formation give an age of 100.3 × 3 Ma and are statistically indistinguishable from biotite grains dated at 103.1 × 3 Ma extracted from the economically important 'Clay Spur' bentonite found at the top of the Mowry Shale. This work provides important new chronometric constraints on a portion of the Medial Jurassic to Late Early Cretaceous stratigraphy of the Big Horn Basin, Wyoming, and may be useful in understanding the regional tectonics that helped shape the development of the Sevier foreland basin and Western Interior Seaway.

  19. Time Evolution of the Basse Terre Island (Guadeloupe, French West Indies) Effusive Volcanism from New K-Ar Cassignol-Gillot Ages.

    Science.gov (United States)

    Samper, A.; Quidelleur, X.; Mollex, D.; Komorowski, J. C.; Boudon, G.

    2004-12-01

    Radiometric dating and geochemistry of effusive volcanics have been combined with geomorphological observations in order to provide a general evolution model of the volcanic island of Basse Terre, Guadeloupe (French West Indies). More than forty new Cassignol-Gillot K-Ar ages distributed within the entire island, together with the twenty ages (Blanc, 1983; Carlut et al., 2000) previously obtained with the same technique, makes the Guadeloupe Island the best place to study the evolution of volcanic processes within the Lesser Antilles Arc. Dating was performed on the carefully separated groundmass in order to avoid K loss due to weathering and excess argon carried by mafic minerals. Ages obtained are relatively younger than previously thought on Basse Terre and range from a few ka to 2.79+-0.04 Ma. When available, the paleomagnetic polarity of the dated flows agree with the GPTS and a very good coherence of ages is observed for each massif. Our results demonstrate the general north to south migration of volcanism through time. It correlates with the main volcanic stages previously identified. The 2.75 Ma Basal Complex, the 1.81+-0.03 _ 1.15+-0.02 Ma Septentrional Chain, the 1.02+-0.02 Ma _ 0.606+-0.02 Ma Axial Chain, the 442+-6 _ 207+-28 ka Mateliane _ Sans Toucher Complex and the basaltic andesites and andesites although a few basalt and dacite have also been dated. All of them are characterized by low MgO values (geochemical characteristics similar to that of the central islands of the Lesser Antilles arc. Within Basse Terre, geochemical characteristics are relatively constant through time, indicating no major change of volcanic processes during the whole subaerial activity. Finally the detailed chronological framework now available provides new constraints for estimating rates of edification and destruction at the island scale and, more generally, to help better understand the evolution of the still active Guadeloupe island Soufriere volcano.

  20. Trombose do seio dural em idade pediátrica

    Directory of Open Access Journals (Sweden)

    Filipe Mira Ferreira

    2015-06-01

    Full Text Available A trombose do seio dural é uma situação clínica rara, que resulta normalmente da complicação de processos infecciosos dos seios perinasais. Os sintomas e sinais são extremamente variados e inespecíficos sendo o diagnóstico feito através da ressonância magnética nuclear. Esse trabalho relata a ocorrência de trombose do seio dural em um paciente com idade pediátrica. Paciente com 10 anos de idade, sexo masculino, foi enviado ao serviço de urgência devido à diplopia e endotropia no olho esquerdo. No exame oftalmológico foi detectado papiledema bilateral, diplopia binocular e endotropia do olho esquerdo. Apresentava acuidade visual de 10/10 bilateralmente. Diante da suspeita de lesão ocupando espaço do sistema nervoso central, foi realizada ressonância magnética nuclear que confirmou o diagnóstico de TSD. Para avaliar a pressão intracraniana foi efetuada uma punção lombar com manometria, e esta demonstrou uma pressão intracraniana de 20mmHg (normal: <15mmHg. Perante isto a criança ficou internada para tratamento médico (enoxaparina de baixo peso molecular 1,5 mg/kg/dia subcutâneo (60 mg/dia, prednisolona 35 mg/dia oral e acetazolamida 250 mg/dia oral durante 10 dias. Após 1 mês de follow-up verificou-se agravamento oftalmológico. A realização de nova punção lombar apresentou uma pressão intracraniana de 40 mmHg que não cedia ao tratamento médico. Após discussão multidisciplinar do caso optou-se pela realização de derivação lombo-peritoneal. A necessidade de uma grande dose de suspeição clínica, tanto para o diagnóstico inicial quanto para a monitorização das complicações, tornam a abordagem da trombose do seio dural um processo singular.

  1. 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...

  2. 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 ...

  3. Efeitos do momento de transferência dos ovos para o nascedouro e da idade da matriz pesada sobre o rendimento de incubação

    OpenAIRE

    V.M. Barbosa; Rocha,J.S.R.; Baião,N.C.; P.M.M. Mendes; M.A. Pompeu; L.J.C. Lara; D.J.A. Miranda; Carvalho,G.B.; Cardoso,D.M.; Cunha, C. E.; Martins,N.R.S.; R.C. Leite

    2013-01-01

    Foram avaliados os efeitos do momento de transferência dos ovos da incubadora para o nascedouro e da idade da matriz pesada sobre o rendimento de incubação. Os tratamentos foram definidos pela idade das matrizes Cobb®, sendo considerados ovos de matrizes novas (33 semanas) e ovos de matrizes velhas (63 semanas), e pelos momentos de transferência da câmara de incubação para os nascedouros (aos 15, 17 e 19 dias). O delineamento experimental foi inteiramente ao acaso em parcelas subdivididas, se...

  4. 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.

  5. Amor, casamento e sexualidade: velhas e novas configurações

    Directory of Open Access Journals (Sweden)

    Maria de Fátima Araújo

    Full Text Available Neste artigo, a autora revisita a história do amor, do casamento e da sexualidade buscando resgatar o processo de construção e transformação das relações amorosas da antigüidade à modernidade. Sua análise enfatiza as mudanças ocorridas no casamento moderno e as novas configurações que adquire na atualidade.

  6. 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...

  7. 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.

  8. 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.

  9. 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.

  10. Violência na Terceira Idade

    OpenAIRE

    Vale, Soraia Domingues

    2014-01-01

    Projecto de Graduação apresentado à Universidade Fernando Pessoa como parte dos requisitos para obtenção do grau de Licenciada em Criminologia No presente projeto, cujo tema é violência sobre os idosos, irão ser definidos, no Capítulo I, conceitos como envelhecimento, violência, tipos de violência, as características das vítimas e dos agressores, fatores de risco e de prevenção e o “estado da arte” sobre o fenómeno da violência na terceira idade. No Capítulo II, são abordados os locais ...

  11. 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.

  12. 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.

  13. 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.

  14. Dating low-grade metamorphism and deformation of the Espinhaço Supergroup in the Chapada Diamantina (Bahia, NE Brazil: a K/Ar fine-fraction study

    Directory of Open Access Journals (Sweden)

    Annette Süssenberger

    Full Text Available This study focuses on the northernmost part of the Mesoproterozoic Espinhaço Supergroup that crops out in the Chapada Diamantina. The fine-fraction K/Ar dating obtained on slightly metamorphosed sediments of the siliciclastic Espinhaço Supergroup shows a polyphase deformation history that corresponds to the Brasiliano (Pan-African orogenic cycle. The isotopic results are interpreted to indicate three age domains coincident with three structurally different domains. Constrained by the Kübler Index ('illite crystallinity' and illite polytypism, the thermal conditions generated during the tectonic activity show a gradual trend from the craton margins to the interior from epizonal to diagenetic. The northern Chapada Diamantina is situated in the foreland of the Riacho do Pontal belt and comprises the sediments of the Espinhaço Supergroup northeast of the Irecê basin. The K/Ar ages for < 2 µm illite fractions range between 645 and 621 Ma [mean 637±9 Ma (2s] and for < 0.2 µm fraction range between 625 and 603 Ma [mean 614±9 Ma (2s]. Samples from the central Chapada Diamantina east of the Irecê basin are not affected by a Brasiliano deformation event and therefore, the N-S-trending structures are assumed to be older. The deformation of the southern Chapada Diamantina was established in conjunction with the formation of the Araçuai orogenesis and the inversion and reactivation of the Paramirim impactogen. The last stage of deformation in this area is recorded by the K/Ar fine-fraction dating between 470 and 460 Ma.

  15. Hidroginástica na terceira idade

    Directory of Open Access Journals (Sweden)

    Karla Campos de Paula

    1998-02-01

    Full Text Available O processo de envelhecimento no indivíduo saudável está relacionado com inúmeras alterações psicológicas e físicas que interferem na área motora, concorrendo para a inatividade e contribuindo para o aparecimento e agravamento de determinadas doenças, além de influenciar negativamente a realização das atividades de vida diária. Portanto, a prática de atividade física é fundamental para o idoso, não só na prevenção de doenças como na reabilitação de suas habilidades motoras, promovendo um estilo de vida saudável que é fator preponderante para a melhoria da qualidade de vida. Contudo, algumas precauções devem ser adotadas na prescrição da atividade direcionada para o idoso, a fim de que esta seja segura e prazerosa. Dentre os exercícios mais adequados aos idosos estão a caminhada, o ciclismo, a natação e a hidroginástica. Devido a sua grande procura, a hidroginástica vem aumentando o número de adeptos na terceira idade. Ela propicia ao idoso o aumento de sua capacidade aeróbia, força muscular, flexibilidade articular e o treinamento de habilidades específicas como equilíbrio e coordenação motora. Soma-se ainda o fato de esta atividade oferecer ambiente de relaxamento e incentivo ao contato social, atuando no combate ao estresse, depressão, na melhoria da autopercepção corporal e da auto-estima. Devemos, então, estar atentos às particularidades da hidroginástica, a fim de aproveitar todas as vantagens que esta oferece para o programa de exercícios direcionado para a terceira idade.

  16. 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.

  17. 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

  18. 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...

  19. Cooling age of the Birimian juvenile crust in West Africa. U-Pb, Rb-Sr and K-Ar data on the 2. 1 Ga granite-greenstone terrains from SW-Niger. Age de refroidissement de la croute juvenile birimienne d'Afrique de l'Ouest. Donnees U-Pb, Rb-Sr et K-Ar sur les formations a 2. 1 Ga du SW-Niger

    Energy Technology Data Exchange (ETDEWEB)

    Lama, C.; Dautel, D.; Zimmermann, J.L. (Centre National de la Recherche Scientifique (CNRS), 54 - Nancy (France). Centre de Recherches Petrographiques et Geochimiques); Barbey, P. (Nancy-1 Univ., 54 (France)); Cheilletz, A. (Centre National de la Recherche Scientifique (CNRS), 54 - Nancy (France). Centre de Recherches Petrographiques et Geochimiques Ecole Nationale Superieure de Geologie Appliquee et de Prospection Miniere, 54 - Nancy (France)); Pons, J. (Orleans Univ., 45 (France))

    1994-08-18

    A comparison between zircon U-Pb, whole-rock Rb-Sr and biotite-amphibole K-Ar data on Birimian granite-greenstone terrains from SW-Niger indicates that the youngest granitic plutons were emplaced at 2.115 [+-] 5 Ma and that both the plutons and the surrounding greenstones yield cooling ages around 2.118 Ma. The age similarity between the end of the plutonism and the cooling of plutons and surrounding greenstone further suggests rapid cooling at the end of the plutonic event and, thus, corroborates a model of greenstone metamorphism linked to the thermal effect of the plutons. (authors).

  20. Pesquisa em saúde, política de saúde e eqüidade na América Latina

    Directory of Open Access Journals (Sweden)

    Alberto Pellegrini Filho

    2004-06-01

    Full Text Available O autor analisa as relações entre pesquisa de saúde, políticas de saúde e eqüidade na América Latina. Descreve novas tendências no modo de produção do conhecimento, que permitem maior integração entre as necessidades sociais e a pesquisa, facilitando o vínculo entre esta e o processo de definição de políticas. Analisa as manifestações das novas tendências na América Latina e finaliza com a descrição de algumas iniciativas promovidas pela OPAS no sentido de aproveitar as oportunidades abertas pelas novas tendências para a melhoria das condições de saúde na região. Busca defender a tese de que a informação e o conhecimento são bens públicos essenciais e que as iniqüidades de acesso a esses bens são importantes determinantes das iniqüidades em saúde. Para que as políticas de saúde e as políticas de pesquisa em saúde se integrem e se consolidem como políticas públicas voltadas a atender ao interesse público e à promoção da eqüidade, é necessário o fortalecimento do processo democrático de definição das mesmas, multiplicando os atores envolvidos, os espaços e oportunidades de interação entre eles e instrumentando sua participação com o acesso eqüitativo a informações e conhecimentos científicos pertinentes que permitam a defesa fundamentada de seus interesses.

  1. Palaeomagnetism and K-Ar and 40Ar/39Ar ages in the Ali Sabieh area (Republic of Djibouti and Ethiopia): constraints on the mechanism of Aden ridge propagation into southeastern Afar during the last 10 Myr

    Science.gov (United States)

    Audin, L.; Quidelleur, X.; Coulié, E.; Courtillot, V.; Gilder, S.; Manighetti, I.; Gillot, P.-Y.; Tapponnier, P.; Kidane, T.

    2004-07-01

    A new detailed palaeomagnetic study of Tertiary volcanics, including extensive K-Ar and 40Ar/39Ar dating, helps constrain the deformation mechanisms related to the opening processes of the Afar depression (Ethiopia and Djibouti). Much of the Afar depression is bounded by 30 Myr old flood basalts and floored by the ca 2 Myr old Stratoid basalts, and evidence for pre-2 Ma deformation processes is accessible only on its borders. K-Ar and 40Ar/39Ar dating of several mineral phases from rhyolitic samples from the Ali Sabieh block shows indistinguishable ages around 20 Myr. These ages can be linked to separation of this block in relation to continental breakup. Different amounts of rotation are found to the north and south of the Holhol fault zone, which cuts across the northern part of the Ali Sabieh block. The southern domain did not record any rotation for the last 8 Myr, whereas the northern domain experienced approximately 12 +/- 9° of clockwise rotation. We propose to link this rotation to the counter-clockwise rotation observed in the Danakil block since 7 Ma. This provides new constraints on the early phases of rifting and opening of the southern Afar depression in connection with the propagation of the Aden ridge. A kinematic model of propagation and transfer of extension within southern Afar is proposed, with particular emphasis on the previously poorly-known period from 10 to 4 Ma.

  2. K-Ar ages of igneous activity in the Amakusa area, Kumamoto prefecture: an investigation of Miocene magmatic activity in the Inner and Outer Zone of Kyushu, southwestern Japan; Kumamotoken Amakusa chiiki no kasei katsudo no K-Ar nendai to Kyushu naitai gaitai ni okeru chushinsei magma katsudo no renji no hikaku

    Energy Technology Data Exchange (ETDEWEB)

    Hamasaki, S. [Geological Survey of Japan, Tsukuba (Japan)

    1997-06-30

    The timing of igneous activity in the Amakusa area, the most southern part of the Inner Zone of Kyushu, was determined on two samples by K-Ar age dating (quartz porphyry: 16.7{+-}0.3 Ma, granodiorite: 14.6{+-}0.3 Ma). These and previous ages indicate that Miocene felsic igneous activity and continuous mafic igneous activity, composed of high Mg andesite, occurred between 19 and 14 Ms. Basalt activity took place at 10 and 7 Ma. The felsic and mafic igneous activity occurred intermittently at 1-3 m.y. intervals in the Amakusa area. Miocene igneous activity was protracted more than 5 m.y. in the Amakusa area and also elsewhere in the Inner Zone of Kyushu, for example, Tsushima (19-14 Ma), Goto (20-7 Ma) and Koshikijima (15-7 Ma). In contrast the ages of Miocene igneous activity in the Outer Zone of Kyushu extend for only about 2 m.y., around 15-13 Ma, which indicates that the range of Miocene magmatic activity in the Inner Zone of Kyushu was longer than that in the Outer Zone. It is possible that different styles of magmatic activity occurred during the Miocene in the Inner and Outer Zone of Kyushu, i.e. back-arc and fore-arc tectonic settings, respectively. In the back-arc area the upper lithosphere expanded, became thin and fractured as a result of being pulled by the subducted lithosphere. After that magma front the asthenosphere ascended intermittently along the cracks in the fractured upper lithosphere, which caused extensive and intermittent magmatic activity. This is one possible explanation why Miocene magmatic activity is protracted in the Inner Zone which was a back-arc area. The Miocene magmatic activity in the Tsushima and Goto area started at 20-18 Ma, which is almost the same time when the Sea of Japan opened. It maybe that a large amount of magmatic activity was associated with the opening of the Sea of Japan at about 20 Ma in the region of the Sea of Japan, Oki, Tsushima and Goto. Magmatic activity in the Goto and Koshikijima

  3. 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?

  4. 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.

  5. Idade pulmonar em mulheres com obesidade mórbida

    Directory of Open Access Journals (Sweden)

    Fabiana Sobral Peixoto-Souza

    2013-06-01

    Full Text Available OBJETIVO: Verificar a influência da obesidade mórbida na idade pulmonar de mulheres e correlacionar com a massa corporal, índice de massa corporal (IMC e variáveis ventilatórias. MÉTODOS: Estudo longitudinal realizado com 72 obesas mórbidas e grupo controle constituído de mulheres eutróficas. As voluntárias realizaram um teste de função pulmonar para determinação da idade pulmonar e os resultados foram correlacionados com as variáveis antropométricas e volumes pulmonares. RESULTADOS: As obesas mórbidas apresentaram uma idade pulmonar significativamente superior (50,1 ± 6,8 anos às eutróficas (38,8 ± 11,4 anos. Não houve diferença entre a idade cronológica entre os grupos. Houve uma correlação significativa e positiva entre idade cronológica, massa corporal e IMC com a idade pulmonar (r = 0,3647, 0,4182, 0,3743, respectivamente. Houve uma correlação negativa entre a capacidade vital forçada (CVF, volume expiratório forçado no primeiro segundo (VEF1, razão (VEF1/CVF e volume de reserva expiratório (VRE com a idade pulmonar (r = -0.7565, -0.8769, -0.2723, -0.2417, respectivamente. CONCLUSÃO: A idade pulmonar das obesas mórbidas encontra-se aumentada e está associada com o aumento da massa corporal e IMC.

  6. Use of combined Hartree–Fock–Roothaan theory in evaluation of lowest states of $K[Ar]4s^0 3d^1$ and $Cr^+ [Ar]4s^0 3d^5$ isoelectronic series over noninteger -Slater type orbitals

    Indian Academy of Sciences (India)

    I I Guseinov; M Erturk; E Sahin

    2011-01-01

    By using noninteger n-Slater type orbitals in combined Hartree–Fock–Roothaan method, self-consistent field calculations of orbital and lowest states energies have been performed for the isoelectronic series of open shell systems $K[Ar]4s^0 3d^1 ({}^2D) (Z = 19–30)$ and $Cr^+[Ar]4s^0 3d^5 ({}^6 S) (Z = 24–30)$. The results of the calculations for the orbital and total energies obtained by using minimal basis-sets of noninteger -Slater type orbitals are given in the tables. The results are compared with the extended-basis Hartree–Fock computations. The orbital and total energies are in good agreement with those presented in the literature. The results can be useful in the study of various properties of heavy atomic systems when the combined Hartree–Fock–Roothaan approach is employed.

  7. K-Ar dating of late Mesozoic volcanism and geochemistry of volcanic gravels in the North Huaiyang Belt, Dabie orogen: Constraints on the stratigraphic framework and exhumation of the northern Dabie orthogneiss complex

    Institute of Scientific and Technical Information of China (English)

    2002-01-01

    Two eruption episodes are identified through systematic field investigations and K-Ar dating of the lateMesozoic volcanic rocks in the North Huaiyang belt (NHB),Dabie orogenic belt, of which the earlier volcanic suitetermed Maotanchang Fm. (Fm.) occurring at Jinzhai,Xianhualing and Maotanchang, etc., was erupted from 149Ma to 138 Ma. The other named Xiaotian Fm. mainly dis-tributed at Xiaotian, Shucheng, etc., was formed between132 Ma and 116 Ma. During the eruption gap of the two vol-canic suites deposited a volcano-sedimentary conglomeratelayer, which are composed of the multi-compositional gravels, including the North Dabie orthogneiss complex (NDOC),volcanic gravels, etc. These volcanic gravels in the con-glomerate layer show identical geochemical and isotopic compositions (87Sr/86Sr(t) =0.7084-0.7092, (Nd (t) = 21.8-24.4) to the Maotanchang Fm. volcanic rocks (87Sr/86Sr = 0.7086-0.7102, (Nd = 19.2-24.4), but significantly distinct from those of Xiaotian Fm. (87Sr/86Sr = 0.7076-0.7084, (Nd = 17.2 - 19.2). K-Ar dating results of its underlying andoverlying volcanic sequences indicate that the conglomerate layers were deposite d at ~135 Ma. This suggests that the NDOC was rapidly exhumed to the surface dur ing or shortly before ~135 Ma and became the important provenance of the late Me sozoic volcano-sedimentary basins in the NHB. In combination with the regional v olcano-sedimentary correlation, we divided the Mesozoic stratigraphic sequence i n the NHB from base to top into Fanghushan Fm. (>160 Ma), Yuantongshan Fm. (/mid dle- lower segment of Sanjianpu Fm.) (160-149 Ma), Maotanchang Fm. (/Zhougongsh an Fm./upper segment of Sanjianpu Fm./Fenghuangtai Fm.) (149-135 Ma) and Xiaoti an Fm. (/Baidafan Fm./Heshidu Fm.) (135-116 Ma).

  8. Mineralogical, chemical and K-Ar isotopic changes in Kreyenhagen Shale whole rocks and <2 μm clay fractions during natural burial and hydrous-pyrolysis experimental maturation

    Science.gov (United States)

    Clauer, N.; Lewan, M. D.; Dolan, M. P.; Chaudhuri, S.; Curtis, J. B.

    2014-04-01

    Progressive maturation of the Eocene Kreyenhagen Shale from the San Joaquin Basin of California was studied by combining mineralogical and chemical analyses with K-Ar dating of whole rocks and bearing minerals of the rocks. The Al/K ratio of the naturally matured rocks is essentially constant for the entire depth sequence, indicating that there is no detectable variation in the crystallo-chemical organization of the K-bearing alumino-silicates with depth. No supply of K from outside of the rock volumes occurred, which indicates a closed-system behavior for it. Conversely, the content of the total organic carbon (TOC) content decreases significantly with burial, based on the progressive increasing Al/TOC ratio of the whole rocks. The initial varied mineralogy and chemistry of the rocks and their sources and depositional settings give scattered results that homogenize progressively during burial due to increased authigenesis, and concomitant increased alteration of the detrital material. Hydrous pyrolysis was intended to alleviate the problem of mineral and chemical variations in initially deposited rocks of naturally matured sequences. However, experiments on aliquots from thermally immature Kreyenhagen Shale outcrop sample did not mimic the results from naturally buried samples. Experiments conducted for 72 h at temperatures from 270 to 365 °C did not induce significant changes at temperatures above 310 °C in the mineralogical composition and K-Ar ages of the rock and heated the most at 365 °C for 216 h. This slight decrease in age outlines some loss of radiogenic 40Ar, together with losses of organic matter as oil, gas, and aqueous organic species. Large amounts of smectite layers in the illite-smectite mixed layers of the pyrolyzed outcrop source rock, the pore system is no longer wetted by water and smectite to illite conversion ceases. Experimental attempts to evaluate the smectite conversion to illite should preferentially use low-TOC rocks to avoid

  9. Cretaceous-Cenozoic tectonic history of the Jiaojia Fault and gold mineralization in the Jiaodong Peninsula, China: constraints from zircon U-Pb, illite K-Ar, and apatite fission track thermochronometry

    Science.gov (United States)

    Deng, Jun; Wang, Changming; Bagas, Leon; Carranza, Emmanuel John M.; Lu, Yongjun

    2015-12-01

    The Jiaojia Fault (JJF) in the Jiaodong area of eastern China is an important NNE-trending structure that is subsidiary to the regional Tancheng-Lujiang (Tan-Lu) Fault Zone, and hosts >1200 t of gold reserves contained in disseminated and stockwork ore, dominantly in the footwall of the fault. We present new zircon U-Pb, apatite fission track, and illite K-Ar data along the JJF and have delineated its tectonic history focusing on its formation and reactivation. Zircon U-Pb dating shows that the Shangzhuang granite is a composite body with ages between 132 ± 1 and 127 ± 1 Ma. Illite K-Ar ages for the fault's gouge range from 83 ± 2 to 68 ± 2 Ma, and the measured apatite fission track ages for ores are between 55 and 21 Ma. Previous zircon U-Pb geochronology and structural studies suggest that the JJF was originally activated in the Jurassic during 160-150 Ma as a sinistral fault. The JJF was a normal fault in the Early Cretaceous due to NW-SE orientated tension and NE-SW compression, which lasted from 135 to 120 Ma. This was followed by sinistral strike-slip faulting due to NW-SE compression and NE-SW tension during 120-110 Ma, and it changed to normal displacement at ca. 110 Ma. Our apatite fission track data analysis and thermal modeling of representative samples suggest that there was a subsequent dextral reactivation of the fault at ca. 55 Ma. Previous age data of ca. 130-110 Ma for gold mineralization along the JJF coincides with the Early Cretaceous magmatism and is coeval with the transition from normal faulting to sinistral strike-slip faulting of the JJF in Early Cretaceous, which is interpreted to be due to changing direction of the subducting Pacific Plate.

  10. 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....

  11. 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....

  12. 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 ...

  13. 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.

  14. 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...

  15. 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 ...

  16. Gastroenterite a shigella na idade pediátrica

    OpenAIRE

    Ferreira, A.; Brito, MJ; Sardinha, T.; Machado, J.; Ferreira, G; Machado, MC

    2003-01-01

    A Shigelose é uma causa importante de morbilidade e mortalidade na idade pediátrica. Objectivos Caracterizar a clínica, epidemiologia e alterações laboratoriais da Shigelose numa população infantil da área Amadora-Sintra e identificar factores associados ao aparecimento de complicações. População e Métodos: Estudo retrospectivo de 1/7/1997 a 30/06/2011 Analisaram-se idade, sexo, raça, condições socio-económicas, contexto epidemiológico, quadro clínico e complicações, exames laborator...

  17. 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.

  18. K-Ar ages of clay-size concentrates from the mineralisation of the Pedroches Batholith, Spain, and evidence for Mesozoic hydrothermal activity associated with the break up of Pangaea

    Energy Technology Data Exchange (ETDEWEB)

    Halliday, A.N. (Scottish Universities Research and Reactor Centre, Glasgow (UK)); Mitchell, J.G. (Newcastle upon Tyne Univ. (UK). School of Physics)

    1984-05-01

    The K-Ar ages of 32 clay concentrates extracted from samples of ore, gangue and wallrock associated with mineralisation in the Pedroches Batholith lie in the range 119-285 Ma. Although some of the mineralisation is of Permian age more than half of the ages lie between 210 and 230 Ma and indicate a hydrothermal event at this (Triassic) time. A comparison with age data for mineralisation and certain anorogenic magmatism in other areas of the North Atlantic reveals a consistent pattern of a major event at ca. 230-210 Ma and a minor event at ca. 160 Ma with little Cretaceous or Tertiary activity. It is proposed that the ca. 230-210 Ma event was related to an initial rapid fracturing of the crust associated with the break up of Pangaea, which was related with an increase in the geothermal gradient and penetration of the deep crust by surface waters which returned via both new and rejuvenated fissure systems.

  19. 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.

  20. 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.

  1. 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.

  2. K-Ar dating and delta O-18-delta D characterization of nanometric illite from Ordovician K-bentonites of the Appalachians: illitization and the Acadian-Alleghenian tectonic activity

    Science.gov (United States)

    Clauer, Norbert; Fallick, Anthony E.; Eberl, Dennis D.; Honty, Miroslav; Huff, Warren D.; Auberti, Amelie

    2013-01-01

    Nanometric (2 diagram that illitization occurred in all fractions by simultaneous nucleation and crystal growth, except for one sample. In that sample, a period of growth without nucleation was detected on top of the nucleation and growth episode. The K-Ar ages organize into two isochrons, the first at 319.9 ± 2.0 Ma with an initial 40Ar/36Ar ratio of 271 ± 66 Ma, and the second at 284.9 ± 1.2 Ma with an initial 40Ar/36Ar ratio of 310 ± 44. One data point above the older isochron and three between the two isochrons suggest a detrital contamination for the former separate and a possible further generation of nanoparticles for the three others. The samples with the older crystallization age consist of illite and illite-rich mixed-layers, and those with the younger age contain smectite-rich mixed-layers without illite, or illite-enriched illite-smectite mixed-layers. The K-Ar ages fit the age trends published previously for similar K-bentonites with regional age patterns between 240 and 270 Ma in the southwestern region, between 270 and 300 Ma in the central zone and the southern Appalachians, and between 315 and 370 Ma in the northernmost. Each of the two generations of illite crystals yields very consistent δ18O (V-SMOW) values at 17 ± 1‰ for the older and at 21 ± 1‰ for the younger. If crystallization temperatures of the nanometric illite were between 100 and 200 °C, as suggested by microthermometric determinations, the hydrothermal fluids had δ18O values of 4 ± 1‰ in the Dalton district and of 8 ± 1‰ in the Lafayette, Trenton, and Dirtseller districts at 100 °C, and of 11 ± 1 and 15 ± 1‰ in the same locations at 200 °C, probably because the water-rock isotope exchanges at elevated temperature occurred in rock-dominated systems. The δ18O of the fluids remained unchanged during local crystal growth, but varied depending on the geographic location of the samples and timing of illitization. The δD (V-SMOW) values of the different size

  3. K-Ar dating, whole-rock and Sr-Nd isotope geochemistry of calc-alkaline volcanic rocks around the Gümüşhane area: implications for post-collisional volcanism in the Eastern Pontides, Northeast Turkey

    Science.gov (United States)

    Aslan, Zafer; Arslan, Mehmet; Temizel, İrfan; Kaygusuz, Abdullah

    2014-04-01

    Volcanic rocks from the Gümüşhane area in the southern part of the Eastern Pontides (NE Turkey) consist mainly of andesitic lava flows associated with tuffs, and rare basaltic dykes. The K-Ar whole-rock dating of these rocks range from 37.62 ± 3.33 Ma (Middle Eocene) to 30.02 ± 2.84 Ma (Early Oligocene) for the andesitic lava flows, but are 15.80 ± 1.71 Ma (Middle Miocene) for the basaltic dykes. Petrochemically, the volcanic rocks are dominantly medium-K calc-alkaline in composition and show enrichment of large ion lithophile elements, as well as depletion of high field strength elements, thus revealing that volcanic rocks evolved from a parental magmas derived from an enriched mantle source. Chondrite-normalized rare-earth element patterns of the volcanic rocks are concave upwards with low- to-medium enrichment (LaCN/LuCN = 3.39 to 12.56), thereby revealing clinopyroxene- and hornblende-dominated fractionations for andesitic-basaltic rocks and tuffs, respectively. The volcanic rocks have low initial 87Sr/86Sr ratios (0.70464 to 0.70494) and ɛNd(i) values (+1.11 to +3.08), with Nd-model ages (TDM) of 0.68 to 1.02 Ga, suggesting an enriched lithospheric mantle source of Proterozoic age. Trace element and isotopic data, as well as the modelling results, show that fractional crystallization and minor assimilation played an important role in the evolution of the volcanic rocks studied. The Eocene to Miocene volcanism in the region has resulted from lithospheric delamination and the associated convective thinning of the mantle, which led to the partial melting of the subduction-metasomatized lithospheric mantle.

  4. Monzonitoid magmatism of the copper-porphyritic Lazurnoe deposit (South Primor'e): U-Pb and K-Ar geochronology and peculiarities of ore-bearing magma genesis by the data of isotopic-geochemical studies

    Science.gov (United States)

    Sakhno, V. G.; Kovalenko, S. V.; Alenicheva, A. A.

    2011-05-01

    Magmatic rocks from the copper-porphyritic Lazurnoe deposit (Central Primor'e) have been studied. It has been found that rocks from the Lazurnyi massif are referred to gabbro-monzodiorites, monzodiorites, and monzo-granodiorites formed during two magmatic phases of different ages. The earlier phase is represented by gabbro-monzodiorites and diorites of the North Stock, and the later one, by gabbro-monzodiorites and monzo-grano-diorites of the South Stock. On the basis of isotopic dating by the U-Pb (SHRIMP) method for zircon and by the K-Ar method for hornblendes and biotites, the age of magmatic rocks is determined at 110 ± 4 for the earlier phase and at 103.5 ± 1.5 for the later one. Examination of the isotopic composition for Nd, Sr, Pb, Hf, δ18O, and REE spectra has shown that melts of the first phase are contaminated with crustal rocks and they are typical for a high degree of secondary alterations. Potassiumfeldspar, biotite, propylitic alterations, and sulfidization are manifested in these rocks. The rocks of the later stage of magmatism are characteristic for a primitive composition of isotopes and the absence of secondary alterations. They carry the features of adakite specifics that allows us to consider them derivatives of mantle generation under high fluid pressure. The intrusion of fluid-saturated melts of the second phase into the magmatic source of the first phase caused both an alteration pattern of rocks and copper-porphyritic mineralization. Isotopes of sulfur and oxygen allow us to consider the ore component to be of magmatic origin.

  5. 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

  6. 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...

  7. 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.

  8. 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

    Directory of Open Access Journals (Sweden)

    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

  9. Concreto submetido a vibrações nas primeiras idades

    Directory of Open Access Journals (Sweden)

    J. F. Fernandes

    Full Text Available Este artigo traz informações sobre o comportamento nas primeiras idades de um concreto de alta resistência, produzido com cimento de alta resistência inicial, lançado e adensado em ambientes submetidos a vibrações, como em obras de pontes de rodovias. Apresenta-se o programa experimental desenvolvido, descrevendo desde a moldagem dos corpos-de-prova, sob ação de vibrações similares às induzidas pelo tráfego, até os ensaios de caracterização mecânica e de aderência aço-concreto. Os resultados experimentais indicam que o concreto submetido à vibração nas primeiras idades pode sofrer perdas na resistência à tração e no módulo de elasticidade. A redução dessas propriedades pode comprometer a utilização da estrutura devido ao aparecimento de flechas e fissuras acima dos limites de norma. A redução da resistência à tração do concreto deve ser considerada, também, na aplicação de pavimentos rígidos, onde essa propriedade é fundamental para garantir a durabilidade do sistema. Não foi observada nenhuma redução na resistência à compressão ou na capacidade de aderência devido à introdução de vibrações nas primeiras idades do concreto.

  10. New K-Ar ages from La Montagne massif, Réunion Island (Indian Ocean), supporting two geomagnetic events in the time period 2.2-2.0 Ma

    Science.gov (United States)

    Quidelleur, X.; Holt, J. W.; Salvany, T.; Bouquerel, H.

    2010-08-01

    We present new radiometric ages obtained at the type locality in La Réunion Island where palaeomagnetic records of the Réunion events have first been identified. Seven dated lava flows from the Rivière Saint Denis section, which recorded a reverse-to-normal transition, display ages from 2.12 +/- 0.03 to 2.17 +/- 0.03 Ma, with a mean age of 2.15 +/- 0.02 Ma. Two significantly younger flows from this section, interpreted here as valley fill flows from trace elements compositions and Pb isotopic data, have been dated at 2.06 +/- 0.03 and 2.08 +/- 0.03 Ma. Within the Grande Chaloupe section, where a normal-to-reverse transition is recorded, two coherent ages of 2.05 +/- 0.03 and 2.03 +/- 0.03 Ma have been obtained. When a direct comparison was possible, our new K-Ar ages performed on separated groundmass show a rather good coherence with previous ages from La Réunion Island. When considered with continuous palaeomagnetic sedimentary records in the 2.2-2.0 Ma interval, these new results suggest that two distinct events are recorded in La Montagne lava flows at La Réunion Island, with ages of 2.15 +/- 0.02 and 2.04 +/- 0.02 Ma. Following recent nomenclature, the former is the Réunion event s.s., while the latter can be related to the Huckleberry Ridge event. Globally distributed volcanic and sedimentary records show that the first (Réunion s.s.; RU-1) is associated with a large dipole intensity decrease at 2.15 +/- 0.02 Ma, and hence is recorded in many sequences. On the other hand, the dipole intensity decrease was not as pronounced at 2.04 +/- 0.02 Ma, when the Huckleberry Ridge (RU-2) palaeomagnetic event occurred. Consequently, it is not present as a full directional change in many sections worldwide, but rather appears as a geomagnetic excursion during an episode of increased secular variation. Finally, the use of the Réunion event for magnetostratigraphic studies is recommended, while the clear identification of the Huckleberry Ridge excursion might often

  11. 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.

  12. 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.

  13. DIVER-IDADES EN LA PSICOGERONTOLOGÍA

    Directory of Open Access Journals (Sweden)

    Graciela Zarebski

    2010-02-01

    Full Text Available La conferencia trata acerca de la continuidad identitaria de nuestra Red Iberoamericana de Psicogerontología, a través de sus congresos: Divers-idades… a partir de la identidad de nuestros viejos… pueblos, que fuera el lema de nuestro primer congreso, pueblos que, en su diversidad, están aquí representados y eso nos lleva a la memoria y construcción de futuro, lema del segundo congreso. De tal modo que se conjugan pasado, presente y futuro en la construcción de un modo de entender y abordar el envejecimiento humano desde la salud mental, tal nuestra especificidad. Por lo tanto, estamos hablando de nuestra identidad, la identidad de la Psicogerontología y de cómo la vamos construyendo através de las diversidades que la componen. Nos ocupamos de sujetos envejecientes y de sus diversos contextos culturales y para hacerlo proponemos un nuevo enfoque en la Psicogerontología –superador del modelo simplista y biologista - desde una perspectiva integradora de los aspectos bio-psico-sociales que complejamente interactúan. En este sentido, la perspectiva de la Teoría del Curso de la Vida que da marco actualmente a la Gerontología, nos instala en las Divers-idades, diversas edades en las cuales favorecer intercambios intergeneracionales y preparación para las vejeces en su divers-idad. El concepto de identidad es central en la Psicogerontología, ya que el envejecer se anticipa como perspectiva de metamorfosis para el yo, el cual ve amenazado, entre otras cosas, su poder. Poder seguir siendo… frente a una cultura que no lo deja ser ni le otorga reconocimiento, dependerá de la construcción de un Yo complejo, en las divers-idades que lo enriquecen. Palabras-clave: Divers-idades. Psicogerontología. Teoría del Curso de la Vida.

  14. Ciclosporina: Riscos em Idade Pediátrica

    OpenAIRE

    Antunes, J.(Laboratório de Instrumentação e Fısica Experimental de Partículas, Lisboa, Portugal); Gouveia, C.; Brito, MJ

    2010-01-01

    Introdução: A eficácia e segurança da ciclosporina têm sido demonstradas em patologias inflamatórias dermatológicas, nomeadamente psoríase e eczema, em adultos e crianças. Na idade pediátrica o seu uso é no entanto ainda limitado. Apresentamos três casos clínicos em que a ciclosporina, foi interrompida por aparecimento de complicações. Este trabalho visa alertar para potenciais efeitos secundários da ciclosporina, a fim de evitar utilizações abusivas. Casos clínicos: Foram submetidas...

  15. 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...

  16. Attempts of whole-rock K/Ar dating of mesozoic volcanic and hypabissal igneous rocks from the Central Subbetic (Southern Spain: A case of differential Argon loss related to very low-grade metamorphism

    Directory of Open Access Journals (Sweden)

    Sanz de Galdeano, C.

    1988-04-01

    Full Text Available 12 samples of basic intrusives within Triassic rocks «ophites» and 11 samples of volcanic and associated intrusives within Jurassic to Early Cretaceous sequences of the Subbetic Zone were subjected to whole-rock K/Ar dating in combination with chemical/petrological analysis. Satisfactory results were obtained only from a number of samples of volcanic rocks, however, analytical ages commonly agree, within about 10 relative percent, with those deduced from stratigraphic location. «Ophite» samples, on the other hand, may reveal considerably lower analytic ages than the volcanics and show much stronger scattering, even among samples collected within a small area. It is argued that the inferred loss of Ar results from very-low-grade alpine metamorphic alteration, which affected the «ophites» more intensely than the higher volcanic rocks. Other post-emplacement chemical changes, such as the degree of secondary oxidation of Fe, are also distintive among the two groups of samples, and are to some extent consistent with the above view in that the alteration environment of the ophites should have produced conditions for more penetrative fluid-rock interactions and homogeneous recrystallization. Overall, the magmatic activity from which the ophitic rocks originated might have started in the Late Triassic and continued in the Lower Jurassic. 80th, the «ophites» and the volcanics are though to be the result of magmatic events Collowing tensional to transtensive crustal movements affecting the external basins of the Betic Cordilleras Crom Late Triassic to Early Cretaceous times.Doce muestras de cuerpos básicos intrusivos en rocas triásicas («ofitas» y 11 muestras de volcanitas y rocas intrusivas asociadas en secuencias jurásico-cretáceas de la zona Subbética han sido objeto de datación radiométrica K/Ar (roca total en combinación con análisis químico-petrográfico. Las edades analíticas obtenidas son 's

  17. O despertar do amor nos bailes da terceira idade

    Directory of Open Access Journals (Sweden)

    Kinas, Rovana

    2010-01-01

    Full Text Available O amor embasa toda forma e relação humana, e por isso, pode ocorrer em todas as idades, sendo uma prova que a velhice pode ser um recomeço. Este estudo discorre sobre como se manifestam as relações amorosas em idosos aposentados frequentadores de bailes da terceira idade. A pesquisa foi do tipo qualitativa, de caráter descritivo exploratória, cujo delineamento foi um estudo de caso realizado com três sujeitos, escolhidos por acessibilidade. Os dados foram coletados por uma entrevista semi-estruturada e analisados através da análise de conteúdo, da qual emergiu sete categorias. Os objetivos da pesquisa foram alcançados: os idosos buscam um relacionamento amoroso pela companhia; o enamoramento pode ser ou não vivenciado como algo satisfatório; e o modo como os relacionamentos se estruturam mostra que todos compartilham tudo, que as mulheres se expressam mais do que o homem, e que o relacionamento pode ser sério quando apoiado pela família

  18. 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

    Directory of Open Access Journals (Sweden)

    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

  19. 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

  20. 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.

  1. Pequenos para idade gestacional: fator de risco para mortalidade neonatal

    Directory of Open Access Journals (Sweden)

    Almeida Márcia Furquim de

    1998-01-01

    Full Text Available OBJETIVO: Estudar as variáveis contempladas na Declaração de Nascimento (DN como possíveis fatores de risco para nascimentos pequenos para a idade gestacional (PIG e o retardo de crescimento intra-uterino como fator de risco para a mortalidade neonatal. MATERIAL E MÉTODO: As variáveis existentes na DN foram obtidas diretamente de prontuários hospitalares. Os dados referem-se a uma coorte de nascimentos obtida por meio da vinculação das declarações de nascimento e óbito, correspondendo a 2.251 nascimentos vivos hospitalares, de mães residentes, ocorridos no Município de Santo André, Região Metropolitana de São Paulo, no período de l/1 a 30/6/1992, e aos óbitos neonatais verificados nessa coorte. RESULTADOS: Obteve-se a proporção de 4,3% de nascimentos PIG, significativamente maior entre os recém-nascidos de pré-termo e pós-termo, entre os nascimentos cujas mães tinham mais de 35 anos de idade e grau de instrução inferior ao primeiro grau completo. Os recém-nascidos PIG apresentam maior risco de morte neonatal que aqueles que não apresentavam sinais de retardo de crescimento intra-uterino. CONCLUSÕES: Em áreas com menor freqüência de baixo peso ao nascer, é importante investigar a presença de retardo de crescimento intra-uterino entre os nascimentos prematuros e não apenas nos nascimentos de termo. O registro da data da última menstruação (ou da idade gestacional em semanas não agregadas na DN facilitaria a detecção de PIGs na população de recém-nascidos.

  2. Structural Relationship Between Piton des Neiges and Piton de la Fournaise Volcanoes: New K-Ar Data and Geomorphological Study of the Takamaka Region (East Reunion Island, Indian Ocean)

    Science.gov (United States)

    Salvany, T.; Lahitte, P.; Gillot, P.; Kluska, J.

    2007-12-01

    Reunion Island (Indian ocean) is a volcanic complex resulting from hotspot activity composed of three coalescent eruptive systems. The first subaerial volcano (la Montagne massif), which only outcrops in the NW part has been dated between 2.2 and 1.8 Ma (McDougall, 1971). After a major flank collapse of this volcano (Gillot et al., 1994), Piton des Neiges (PNv) edificated from 1.2 Ma to 30 ka (McDougall., 1971; Gillot et al.,1982). then, Piton de la Fournaise volcano (PFv), one of the most active on Earth, started its activity about 530 kyr ago (Gillot et al., 1989; 1990) and was affected by 3 eastward flank collapses (Gillot et al., 1994). Its present complex morphology is characterized by large scale erosional depressions, (Cirques) cut in the volcanic structures, such as Cilaos, Mafate or Salazie in PNv, Grand Bassin between the two volcanoes, and Grand Pays in PFv. Due to the tropical conditions, deeply incised valleys are present throughout the island. The eastern part of the island (Takamaka area), where we show that products of both PNv and PFv overlap, is one of the most rainy place in the world. It is deeply incised and has been highly eroded during the coeval building stages of PFv and PNv since at least 530 kyr. In order to constrain the relationship between the PNv and PFv volcanoes and to characterise the morphological evolution of this area, we realized a new geochronological study of the different massifs based on the accurate K- Ar technique devoted to the dating of very young rocks (Cassignol technique; Gillot et Cornette, 1986). A preserved structure between the two volcano, Morne de l'Etang, is dated between 1.36 +/- 0.02 Ma, which is older than the primary known activity of Piton des Neiges (about 1.2 Ma; McDougall, 1971), to 0.97 +/- 0.02 Ma. It may either correspond to a remnant and older part of PNv or it belongs to the Proto Fournaise 'les Alizés' volcano', which existence is still debated. Our analysis also emphasizes the fact that PFv

  3. 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

  4. Traumatismos cranianos na idade avançada

    Directory of Open Access Journals (Sweden)

    G. Lausberg

    1974-06-01

    Full Text Available Relato dos aspectos clínicos apresentados por 299 pacientes com mais de 50 anos de idade, que sofreram traumatismos cranianos. Em especial são abordadas as dificuldades no diagnóstico diferencial que os hematomas intracranianos apresentam nesse grupo etário (total de 42 casos. Complicações cerebrais e extra-cerebrais, isto é, extra-cranianas são discutidas, tendo-se especial cuidado nos casos com inconsciência secundária e/ou sinais neurológicos secundários. Comparação com grupos mais jovens é feita. São salientadas as medidas terapêuticas gerais que podem diminuir a alta quota de mortalidade.

  5. Mutismo Selectivo: da Infância à Idade Adulta

    OpenAIRE

    Araújo, A; Hanemman, S

    2011-01-01

    Introdução: O mutismo selectivo (MS) é um distúrbio da comunicação, caracterizado por incapacidade persistente em falar em situações sociais específicas apesar do discurso fluente ser possível noutras circunstâncias. A prevalência estimada é de 0,7 a 2%, sendo habitualmente identificado entre os 6-8 anos de idade. É ligeiramente mais frequente no sexo feminino (ratio feminino:masculino 1,2:1). A duração varia de alguns meses até vários anos, embora na maioria dos casos se observe remissão ...

  6. 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.

  7. 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...

  8. 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...

  9. Qualidade da educação universitária: isomorfismo, diversidade e eqüidade

    Directory of Open Access Journals (Sweden)

    Marília Costa Morosini

    2001-08-01

    Full Text Available As tendências internacionais trazidas pela idade do conhecimento, acirradas pela internacionalização e pelo desenvolvimento de novas tecnologias de comunicação, têm disseminado, marcadamente, entre nós, país caracterizado historicamente pela controle do Estado sobre a educação superior, a era da qualidade. Este trabalho examina diferentes concepções e estratégias de qualidade universitária, advindas de experiências internacionais. Entre os principais conceitos destacam-se o de qualidade, sinônimo de isomorfismo, refletindo-se como avaliação institucional estandartizada e empregabilidade; qualidade, sinônimo de respeito às especificidades; e qualidade, sinônimo de equidade. Pela escassez de bibliografia quanto a uma visão holística do tema, este trabalho, mais do que apresentar propostas, levanta questionamentos quanto à relação entre qualidade e inovação educativa e unicidade do conceito de qualidade e a realidade brasileira.

  10. As estratégias empresariais e a exclusão por idade

    Directory of Open Access Journals (Sweden)

    Marcos Augusto de Castro Peres

    2007-12-01

    Full Text Available Este artigo analisa os elementos de exclusão por idade presentes nas estratégias empresariais e nos processos de seleção profissional. Procuramos demonstrar que os limites de idade que integram o perfil dos cargos a serem preenchidos e os elementos de exclusão presentes nos novos paradigmas produtivos representam uma clara discriminação contra os trabalhadores mais velhos. Neste trabalho, propomos um estudo sobre tais elementos, no intento de demonstrar que os limites de idade ferem o princípio da eqüidade, apoiado na igualdade de oportunidades, com base em anúncios de emprego contendo limites de idade, em bibliografia específica sobre desemprego e exclusão no trabalho, e em dados estatísticos sobre a queda da faixa de idade nos cargos de gerência.

  11. 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 ...

  12. 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.

  13. 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

  14. 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

  15. Grupo Feliz Idade: cuidado de enfermagem para a promoção da saúde na terceira idade

    OpenAIRE

    Victor,Janaína Fonseca; Vasconcelos,Francisca de Fátima; Araújo,Adriana Rocha de; Ximenes,Lorena Barbosa; Araújo,Thelma Leite de

    2007-01-01

    Este artigo teve como objetivos relatar a experiência da formação do grupo de idosos Feliz Idade, desenvolvido por enfermeiras do Programa Saúde da Família em Fortaleza-CE, bem como conhecer a importância do cuidado de enfermagem para a promoção da saúde na vida dos idosos. A seleção inicial dos participantes do grupo ocorreu entre os 314 idosos pertencentes aos programas de Hipertensão Arterial e Diabetes Mellitus. Para formação do grupo, as enfermeiras contaram com a colaboração de médico, ...

  16. 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

  17. 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...

  18. 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.

  19. 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.

  20. 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.

  1. 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

  2. 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

  3. 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

  4. 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...

  5. 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.

  6. 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.

  7. 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.

  8. 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.

  9. Uma proposta de dança na melhor idade

    Directory of Open Access Journals (Sweden)

    2006-11-01

    Full Text Available O presente trabalho relata experiência vivenciada no programa “Começar de Novo”, uma proposta metodológica de dança na maturidade. O programa visa desenvolver ações socioeducativas, artístico-integrativas, através de processos interdisciplinares entre as áreas da dança, música e artes plásticas. Propusemos uma construção coletiva de aulas e proposições coreográficas, visando a uma reflexão sobre a arte na maturidade, as possibilidades da expressão de cada aluno, e também um debate sobre o corpo maduro, suas mudanças e conquistas e a experimentação do fazer e do fruir artístico. PALAVRAS-CHAVE: Dança - Maturidade - Terceira Idade. This paper describes the experience of program “Começar de Novo” (To Start Over Anew, a methodological proposal of Dancing in the maturity. The program aims at developing socio-educational procedures through interdisciplinary activities among the fields of Dancing, Music and Art. A collective planning of the classes and of choreographic propositions was suggested seeking a reflection upon art in the old age, the possibilities of each students`s expression, as well as a debate about the mature body, its changes and conquests and the experience of making and finding pleasure in art. KEYWORDS: Dancing - Maturity - The Third Age.

  10. Qualidade da carne de frangos caipiras abatidos em diferentes idades

    Directory of Open Access Journals (Sweden)

    X.R. Souza

    2012-04-01

    Full Text Available Neste trabalho, foram avaliadas as características físico-químicas e de composição centesimal da carne de frangos machos de três linhagens utilizadas para criação semi-intensiva: Redbro Cou Nu - Vermelho de Pescoço Pelado (Pescoço Pelado; Redbro Plumé - Vermelho de Pescoço Emplumado (Pesadão e Gris Barre Plumé (Carijó. Foram analisadas diferenças em relação à linhagem e à idade de abate (70, 85 e 110 dias. Na carne do peito, não foi verificado efeito de linhagem sobre os parâmetros de cor (L*, a* e b* e pH final. Houve comportamento diferenciado para as aves em relação a qualidade da carne do peito, com menores valores de maciez para linhagem Pesadão e de Perda de Peso por Cozimento para linhagem Carijó. A linhagem Carijó apresentou, para a carne de peito aos 110 dias, os menores valores de umidade e as maiores médias de proteína. Os valores de proteina reduziram para linhagem Pescoço Pelado a partir de 85 dias. Na coxa, a partir de 110 dias, foi verificada redução dos valores de L* (luminosidade e aumento das médias de a* (vermelho. Os valores de força de cisalhamento e extrato etéreo aumentaram para peito e coxa a partir dos 110 dias. As linhagens Pesadão e Pescoço Pelado apresentaram de forma geral, melhores aspectos físico-quimicos, que são os atributos de maior preferência pelo consumidor em função deste tipo de produto.

  11. 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

  12. 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

  13. 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...

  14. 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.

  15. 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...

  16. 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.

  17. 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.

  18. Prevalência de tontura na terceira idade

    Directory of Open Access Journals (Sweden)

    Lidiane Maria de Brito Macedo Ferreira

    2014-06-01

    Full Text Available Objetivo aferir a prevalência de tontura em idosos participantes de um grupo de convivência do Sistema Único de Saúde localizado em centro de especialidades e assistência à saúde do idoso no município de Natal-RN. Métodos estudo prospectivo. Para estatística, utilizou-se análise descritiva dos dados. Resultados foram entrevistados 50 idosos, com idades entre 60 e 88 anos. A prevalência de tontura nesta população foi de 74%. Destes, 35,1% apresentavam apenas vertigem; 13,5% apresentavam vertigem associada a outro tipo de tontura; 24,3% apresentavam desequilíbrio; 8,1% flutuação; 16,2% pré-síncope; e 2,7% flutuação e pré-síncope. Em relação à duração da tontura, 48,6% tinham duração de segundos. Quanto à presença de sintomas otoneurológicos associados, 48,64% referiram sintomas neurovegetativos, 56,8% tinham zumbido, 56,8% apresentavam hipoacusia e 43,2% apresentavam plenitude aural. Referente a outras alterações, 10,8% não usava óculos; 2,7% usavam aparelho auditivo e 8,1% usavam bengalas, 48% tinham 2 ou mais doenças associadas e 40% faziam uso de 3 ou mais medicamentos ao dia. Comparando-se os pacientes com tontura e os sem tontura, achou-se RP de 0,947 para número de comorbidades e 0,971 para número de medicamentos. Na comparação entre idosos com vertigem e outros tipos de tontura, achou-se RP de 1,197 para zumbido, 1,050 para plenitude aural, 2,111 para sintomas neurovegetativos, 0,480 para duração da tontura, 0,528 para número de comorbidades e 0,758 para número de medicamentos. Conclusão conclui-se que a tontura é um sintoma bastante prevalente no idoso da comunidade assim como a presença de co-morbidades e uso de vários medicamentos.

  19. 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.

  20. 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.

  1. /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.

  2. 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...

  3. 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.

  4. 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.

  5. 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...

  6. Desenvolvimento das universidades e bibliotecas universitárias na Idade Média até à Modernidade

    Directory of Open Access Journals (Sweden)

    Fabiene Castelo Branco Diógenes

    2017-01-01

    Full Text Available O artigo analisa a origem das universidades, suas lutas pela autonomia, organização das estruturas administrativa e curricular e relata a existência das bibliotecas ligadas às universidades, desde a Idade Média até a Modernidade. No século XIX a educação é assumida pelo Estado, criando uma cobertura legal que garante às universidades a liberdade científica e pedagógica. A biblioteca universitária teve o seu desenvolvimento ao longo dos séculos, tentando acompanhar essas mudanças. Mas, é no decorrer desse século que alguns serviços e foram surgindo os entendimentos da relação da biblioteca com a universidade. Entretanto, foi a partir da Segunda Guerra que o ensino começa a ter característica de atividade de massa, e a biblioteca universitária se torna uma parte importante na universidade. Cresce a ênfase ao acesso às coleções, há financiamento do Estado para desenvolvimento de coleções e estruturação de suas bibliotecas, dão-se início às atividades de cooperação e de automação. Estas começam a mudar a forma como são oferecidos os serviços e produtos das bibliotecas universitárias. A partir de 1970, as novas tecnologias penetram nessas áreas, e as universidades e suas bibliotecas são afetadas por tais tecnologias. Propostas de reformas surgem gerando novos desafios para estas duas instituições centenárias.

  7. U/Pb (SHRIMP), {sup 207}Pb/{sup 206}Pb, Rb/Sr, Sm/Nd e K/Ar geochronology of granite-greenstone terrains of Gaviao Block: implications for the Proterozoic and Archean evolution of Sao Francisco Craton, Brazil; Geocronologia U/Pb (SHRIMP), {sup 207}Pb/{sup 206}Pb, Rb/Sr, Sm/Nd e K/Ar dos terrenos granito-greenstone do Bloco do Gaviao: implicacoes para a evolucao arqueana e proterozoica do craton do Sao Francisco, Brasil

    Energy Technology Data Exchange (ETDEWEB)

    Leal, Luiz Rogerio Bastos

    1998-07-01

    The Gaviao Block (GB) in the northern portion of the Sao Francisco Craton-Northeast of Brazil, constitutes one of the oldest Archean fragments of the South American Platform Archean crust. GB underwent several events of juvenile accretion and reworking of continental crust along its evolutionary history, notably between the Archean and the Paleoproterozoic. {sup 207}Pb/{sup 206}Pb isotopic analyses were carried out in two zircons populations from strongly migmatized TTG terranes found in the proximity of Brumado: the first population (7 crystals) is taken as representative of the crystallization period of the TTG terranes at 3300 {+-} 45 Ma; the second (2 crystals) represents the age of the first even of metamorphism/migmatization at 2910 {+-} 10 Ma. {sup 207} Pb/{sup 206} Pb analyses in zircons from an outcrop of non-migmatized TTG in the area yielded a 3202 {+-} 15 Ma age (4 crystals), interpreted to be the crystallization period of the gneiss protolith. Sm/Nd analyses on the TTG rocks of the Brumado region yielded T{sub DM} model ages varying between 3.26 and 3.36 Ga and {epsilon}{sub Nd}{sup (t)} between -3.5 and +0.7. These data suggest the occurrence of juvenile accretions to the continental crust during the Archean, with differential involvement of crustal materials. The geochemical data of rare earth elements corresponding to the TTG terranes revealed moderate LRRE contents (La{sub N}=83,5), low HREE contents (La{sub N}=2,5) and a fairly fractionated pattern (La/Yb){sub N}=34, besides lack of negative Eu anomaly, showing that these rocks have similar compositions to those TTG terranes of cratonic continents, as well as some Archean rocks from CSF (e.g. Sete Voltas, Boa Vista). Finally, the youngest ages present in GB rocks (ca. 1.2-0.45 Ga) represent the role played by tectono thermal events, which produced partial or total rejuvenation of the Rb/Sr and K/Ar isotopic systems during the Espinhaco and Brasiliano cycles. In particular, K/Ar ages illustrate the

  8. 塔里木盆地典型砂岩油气储层自生伊利石K-Ar同位素测年研究与成藏年代探讨%K-Ar Dating of Authigenic Illites and Its Applications to the Study of Hydrocarbon Charging Histories of Typical Sandstone Reservoirs in Tarim Basin, China

    Institute of Scientific and Technical Information of China (English)

    2005-01-01

    The Tarim Basin in China comprises eight sets of sandstone reservoirs, five of which are investigated in detail in this study. The main purpose of this study is to investigate the hydrocarbon charging histories of reservoirs by applying K-Ar dating of authigenic illites. The ages of authigenic illites from the Lower Silurian bituminous sandstones in the Central Uplift area range from 383.5 to 235.2 Ma, suggesting that the Silurian oil accumulations were formed from the late Caledonian till the late Hercynian. The ages of authigenic illites from the Upper Devonian Donghe Sandstone reservoirs range from 263.8 to 231.3 Ma, indicating that hydrocarbon accumulations within the Donghe sandstone were formed mainly in the late Hercynian. The authigenic illites ages from the Lower Jurassic Yangxia Group sandstones in the Yinan-2 gas reservoir (Yinan-2, Kuqa Depression) range from 28.1 to 23.9 Ma, suggesting that the initial hydrocarbon charging occurred in the Miocene. The ages of the authigenic illites from the Lower Cretaceous sandstones in the Akemomu gas field (Ake-1, Kashi Sag, Southwest Depression) range from 22.6 to 18.8 Ma, indicating a probable early oil accumulation or early migration of hydrocarbon within this area. The illites from the Paleogene sandstones in the Dina-2 gas reservoir (Dina-201, Kuqa Depression) have a detrital origin; they cannot be used to study the hydrocarbon charging histories. The ages of authigenic illites in the underlying Cretaceous sandstones in the same well (Dina-201)range from 25.5 to 15.5 Ma, indicating that hydrocarbon charging in this reservoir probably occurred within the Miocene.This study highlights the potential of applying K-Ar dating of authigenic illites to investigate the timing of hydrocarbon charging histories of the Tarim Basin reservoir sandstones.

  9. 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....

  10. 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.

  11. 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.

  12. 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...

  13. 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.

  14. 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.

  15. 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.

  16. 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...

  17. 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.

  18. 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...

  19. 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.

  20. 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...

  1. 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

  2. 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

  3. 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…

  4. 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:

  5. 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.

  6. 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...

  7. 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 ...

  8. Composição química de genótipos de cana-de-açúcar em duas idades, para fins de nutrição animal Chemical composition of sugarcane in two ages, for animal nutrition

    Directory of Open Access Journals (Sweden)

    João Batista de Andrade

    2004-12-01

    Full Text Available Foi desenvolvido, em 1999/2000, no Instituto de Zootecnia, em Nova Odessa (SP, um experimento para avaliar 60 genótipos de cana-de-açúcar (24 cultivares e 36 clones, para fins de alimentação animal. O experimento foi executado em delineamento de blocos ao acaso, com três repetições. Os genótipos foram amostrados aos 12 e 18 meses de idade. Para todas as características analisadas: porcentagem de matéria seca (%MS; de proteína bruta (%PB; de extrato etéreo (%EE; de matéria mineral (%MM; de carboidratos totais não estruturais (%CTN; de fibra insolúvel em detergente neutro (%FDN; de fibra insolúvel em detergente ácido (%FDA; de celulose (%CEL; de hemicelulose (%HEM; de lignina (%LIG, verificaram-se diferenças entre os genótipos e as idades de corte, com exceção para %EE, que não mostrou diferença entre as idades de corte. Para (%CTN, %NDF, %ADF, %CEL, %HEM e %LIG foram observadas diferenças dos genótipos nas idades de corte.At the Instituto de Zootecnia, Nova Odessa (SP, Brazil, it was carried out an experiment to evaluate 24 cultivars and 36 sugarcane clones as raw material for animal feeding. The experimental design was set in randomized blocks with three replications. The sugarcanes were harvested at 12 and 18 months. Genotypes and age of harvest showed differences for %DM (dry matter; %CP (crude protein; %EE (ether extract; %ACH (ach; %TNC (total non-structural carbohydrates , %NDF (neutral detergent fiber; %ADF (acid detergent fiber; %CEL (cellulose; %HCEL (hemicellulose and %LIG (lignin, except for %EE, for harvest ages. Significant differences for %TNC, %NDF, %ADF, %CEL, %HCEL and %LIG were observed for two ages of harvest.

  9. 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.

  10. Capacidade atencional: há decréscimo como passar da idade?

    Directory of Open Access Journals (Sweden)

    Fabián Javier Marín Rueda

    Full Text Available O objetivo do estudo foi procurar evidência de validade baseada na variável idade para o Teste de Atenção Alternada - TEALT. Para isso, foi verificado se a capacidade de alternar a atenção diminuiria com o passar da idade. Participaram 798 indivíduos, dos Estados da Bahia e de Sergipe, sendo 442 (55,4% da Bahia e 356 (44,6% de Sergipe, do sexo masculino e feminino, e com idades variando entre 18 e 72 anos (M=26,56, DP=8,30. Em Sergipe, os participantes foram estudantes universitários de diferentes cursos, e, na Bahia, foram pessoas que passaram pela avaliação psicológica para a obtenção da carteira de motorista. O TEALT foi aplicado coletivamente no Estado de Sergipe, e de forma individual na Bahia. Os resultados evidenciaram correlação negativa e significativa entre a pontuação do TEALT e a idade, sendo formadas três faixas etárias que se diferenciaram no desempenho no teste. Dessa forma, concluiu-se por evidência de validade para o TEALT em função da idade, sendo que o seu aumento correspondeu a uma diminuição da capacidade de atenção alternada.

  11. 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...

  12. 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

  13. 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.

  14. 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.

  15. 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.

  16. 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.

  17. 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.

  18. 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.

  19. Influência da idade dos ovos de Oxydia vesulia no parasitismo de Trichogramma maxacalii.

    OpenAIRE

    Oliveira Harley Nonato de; Pratissoli Dirceu; Zanuncio José Cola; Serrão José Eduardo

    2003-01-01

    Trichogramma é um dos gêneros de insetos mais importantes no controle biológico. Este trabalho avaliou o potencial de parasitismo de Trichogramma maxacalii em ovos de Oxydia vesulia, em diferentes estágios embrionários. Vinte e cinco ovos de O. vesulia, com um, três, cinco e sete dias de idade foram oferecidos a uma fêmea de T. maxacalii, em ensaio com 15 repetições, por um período de 24 horas. Não houve influência da idade dos ovos de O. vesulia na porcentagem de parasitismo, na viabilidade,...

  20. 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 ...

  1. 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.

  2. 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

  3. 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.

  4. Idade dos ratos versus idade humana: qual é a relação? Rat's age versus human's age: what is the relationship?

    Directory of Open Access Journals (Sweden)

    Nelson Adami Andreollo

    2012-03-01

    Full Text Available RACIONAL: Milhões de ratos são empregados anualmente em pesquisas e no ensino. A exata relação entre a idade dos ratos, comparada com a idade dos humanos ainda é assunto de discussão e controvérsias. OBJETIVO: É revisar a literatura, analisando a idade dos ratos em comparação com a idade dos homens. MÉTODOS: Foram revisadas as publicações existentes sobre o assunto contidas nas bases Medline/Pubmed, Scielo, Biblioteca Cochrane e Lilacs cruzando os descritores ratos, cirurgia experimental e fisiologia. RESULTADOS: Ratos desenvolvem rapidamente durante a infância e se tornam sexualmente maduros com cerca de seis semanas de idade, mas atingem a maturidade social cinco a seis meses mais tarde. Na idade adulta, a cada mês do animal é aproximadamente equivalente a 2,5 anos humanos. Vários autores realizaram trabalhos experimentais em ratos e afirmaram existir correspondência de 30 dias de vida do homem para cada dia de vida do rato. CONCLUSÃO: As diferenças na anatomia, fisiologia, desenvolvimento e fenômenos biológicos devem ser levados em consideração quando são analisados os resultados de qualquer pesquisa em ratos em que a idade é um fator crucial. Cuidado especial é necessário ser tomado quando os estudos efetuados pretendem produzir correlação com a vida humana. Para isso, atenção especial é necessária para verificar a fase em dias do animal e sua correlação com os anos em humanos.BACKGROUND: Millions of mice are used annually in research and teaching. The exact relationship between age of the animals compared with the age of humans is still subject to discussion and controversy. OBJECTIVE: Literature review analyzing the age of rats in comparison with men age. METHODS: Were reviewed the existing publications on the subject contained in Medline / Pubmed, Scielo, The Cochrane Database of Systematic Reviews and Lilacs crossing the headings rats, experimental surgery and physiology. RESULTS: Rats rapidly develop

  5. 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.

  6. 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....

  7. 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.

  8. 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.

  9. 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...

  10. 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...

  11. Imunidade celular em caninos neonatos - do nascimento ao 45° dia de idade

    Directory of Open Access Journals (Sweden)

    R.P. Klein

    2014-06-01

    Full Text Available O objetivo do presente trabalho foi acompanhar o desenvolvimento imunológico dos neonatos caninos, a fim de avaliar a imunidade celular pela análise dos leucócitos e linfócitos totais e das subpopulações de linfócitos T (CD4+ e CD8+ pela técnica de citometria de fluxo. Foram utilizados 30 cães neonatos de ambos os sexos, sem raça definida, aos três, 10, 17, 24, 31, 38 e 45 dias de idade. A contagem de leucócitos totais aos 45 dias (11.639±3.574 foi significativamente maior que no terceiro dia de idade (8.740±1.812 (P<0,05; não houve diferença entre a contagem total de linfócitos aos 45 dias em relação ao terceiro dia de idade. Quanto às subpopulações de LT CD4+ e LT CD8+, os percentuais de LT CD4+, aos três dias de idade (24,9±16,8%, foram inferiores quando comparados à média entre o 10°, o 24° e o 31°dia (35,5%, e os de CD8+, ao terceiro dia, menores em relação às médias do 10° e do 31° dia de idade. Pode-se concluir que as subpopulações de LT CD4+ e CD8+ sofrem oscilações durante o desenvolvimento pós-natal, sendo estas crescentes em relação aos níveis obtidos aos três dias de idade. A relação CD4+:CD8+ mostrou superioridade para o primeiro tipo celular, sendo que a maior relação entre CD4+ e CD8+ ocorreu no terceiro dia de idade. Com base nos resultados obtidos neste estudo, notaram-se as diferenças semanais nas populações linfocitárias, o que demonstra a dinâmica dessas células durante o período neonatal.

  12. 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...

  13. 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.

  14. 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...

  15. 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.

  16. 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.

  17. 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.

  18. 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.

  19. 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).

  20. 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...

  1. 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.

  2. 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....

  3. 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...

  4. 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.

  5. 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.

  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. O jogo e a timidez em crianças em idade pré-escolar

    OpenAIRE

    Valente, Regina Feliciano

    2014-01-01

    Dissertação de mestrado, Educação Pré-Escolar, Escola Superior de Educação e Comunicação, Universidade do Algarve, 2014 O presente relatório incide sobre o jogo e a timidez em crianças em idade pré escolar e desenvolveu-se no âmbito da prática de ensino supervisionada (PES), que decorreu num jardim de infância em Faro, junto de um grupo de 14 crianças com idades compreendidas entre os 5 e 6 anos. No presente estudo, de cariz quantitativo, tivemos como principal objetivo identificar e co...

  8. Elementos sobre a concepção de Meia-Idade no processo de envelhecimento

    Directory of Open Access Journals (Sweden)

    Priscilla de Cesaro Antunes

    2014-03-01

    Full Text Available Este ensaio visa a apresentar elementos que contribuam no entendimento da concepção de Meia-Idade, conceito que diz de um momento de vida mais específico dentro do intervalo chamado idade adulta. Discute evidências de uma simplificação conceitual com tendência à homogeneização de comportamentos, condições e necessidades dessas pessoas, além de indicações sobre o trato com categorias geracionais e uma possível conceituação. Problematiza a ênfase na aparência corporal na contemporaneidade, diante da negação do envelhecimento.

  9. 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.

  10. Nível de atividade física, comorbidades e idade de pacientes hipertensos

    Directory of Open Access Journals (Sweden)

    Denise Rodrigues Bueno

    2013-09-01

    Full Text Available No envelhecimento, hábito inativo está associado a doenças crônicas. Existem diferentes domínios da atividade física, tais como: tempo livre e locomoção. O objetivo foi analisar associações entre diferentes domínios de atividade física, comorbidades e idade em hipertensos. Foram entrevistados 192 hipertensos. Classificados em menos ativos e mais ativos para atividades no lazer, locomoção, ocupação e total e estratificados em grupos etários. A circunferência de cintura foi avaliada e comorbidades auto referidas. O teste Qui-quadrado analisou as associações e o teste ANOVA one way comparou os grupos etários, adotando significância estatística quando p<0,05. As médias de atividade física ocupacional e total foram menores para idade igual ou acima dos 60 e 70 anos, respectivamente. A atividade ocupacional esteve associada à idade em mulheres e, ao colesterol e diabetes em homens, que também tiveram atividade física de locomoção associada à circunferência de cintura. Em síntese a atividade física de hipertensos associa-se a comorbidades para diferentes grupos etários e sexos.

  11. 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...

  12. 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.

  13. 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.

  14. A Nova Filantropia Capitalista e a Intensificação do Trabalho Docente - reflexões sobre o voluntariado empresarial

    Directory of Open Access Journals (Sweden)

    Maria Vieira Silva

    2012-04-01

    Full Text Available O texto sintetiza resultados de pesquisas dos autores sobre os novos formatos da filantropia capitalista por meio do trabalho voluntário. Coloca em relevo, especificamente, práticas pedagógicas desenvolvidas no âmbito das empresas com “responsabilidade social” consolidando uma nova modalidade de trabalho docente. A partir dos discursos dos gestores da empresa e dos docentes voluntários as análises problematizam os paradoxos, contradições e ambigüidades presentes nas ações voluntárias, apreendendo os processos de intensificação laboral presente no conjunto dos mecanismos da administração capitalista, os quais incidem sobre as dimensões subjetivas do trabalhador e nas dimensões objetivas de ampliação do capital.

  15. Artesanato na terceira idade: um estudo na cidade de Sinop no ano de 2011

    Directory of Open Access Journals (Sweden)

    Rosane Marlene Weber

    2015-04-01

    Full Text Available Essa pesquisa tem como objetivo mostrar a importância do artesanato na Terceira Idade como atividade educacional e de autonomia para os idosos. Por existir uma preocupação com a qualidade de vida da Terceira Idade e sua autonomia, nesta fase que muitos acabam ficando dependentes dos membros da família, espera-se encontrar através da arte uma motivação e uma forma de demonstrar a autoria por meio do fazer, criar e recriar com o artesanato. Aprender e ensinar são um processo contínuo na vida do ser humano, independente da idade, para Paulo Freire precisamos ter consciência de que somos inacabados, e sendo conscientes de nossa inconclusão, devemos viver num permanente movimento de busca. Essa é uma das causas pelas quais será pesquisada a prática formativa/educacional por meio do artesanato na Terceira Idade. Os motivos que levaram a escolha desta pesquisa com o artesanato na Terceira Idade é o fato de ter vivido uma experiência de trabalho na ala geriátrica de um hospital. Já o artesanato é a arte que fascina, e acreditamos que sempre há tempo para recomeçar, para descobrir algo que possa trazer qualidade para nossa vida. Devido ao crescimento cada vez maior da expectativa de vida em nosso país, cria-se uma preocupação com a qualidade de vida das pessoas da Terceira Idade. Em relação aos aspectos educacionais e culturais, esta pesquisa deseja compreender como o artesanato pode trazer motivação para as pessoas da Terceira Idade como forma de autoria e autonomia, nesta fase da vida, na cidade de Sinop, e quais os motivos que os levam a realizar esse tipo de atividade. Para investigação teórica desta pesquisa do Artesanato na Terceira Idade: um estudo na cidade de Sinop em 2011 usaremos bibliografia de vários autores, mas em especial os que dedicam seus estudos a esta faixa etária, como a coleção de Vivaidade, que tem como organizadora principal Anita Liberalesso Neri. Os autores desta coleção nos trazem a reflex

  16. 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...

  17. 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...

  18. 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-...

  19. 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.

  20. 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

  1. 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.

  2. 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.

  3. 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

  4. 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.

  5. 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 .

  6. 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.

  7. 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.

  8. 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.

  9. 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…

  10. 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…

  11. 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...

  12. 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.

  13. Representações sociais da participação em atividades de lazer em grupos de terceira idade

    Directory of Open Access Journals (Sweden)

    Maria Lúcia Olivetti Borini

    2002-10-01

    Full Text Available O objetivo da pesquisa é estudar as representações sociais acerca da participação em atividades de lazer nos grupos de Terceira Idade. Foram realizadas treze entrevistas individuais com participantes homens e mulheres, com idade superior à 60 anos, em um Centro de Convivência para a Terceira Idade. Os discursos foram analisados a partir da técnica de análise de conteúdo e à luz da Teoria das Representações Sociais. As "marcas da velhice" como a falta de atividades, solidão e as doenças são os motivos que levam os idosos a freqüentarem as atividades de lazer no Centro de Convivência para a Terceira Idade. Eles revelam pertencerem à "família da Terceira Idade" e encontram um "efeito terapêutico" para as "marcas da velhice". Participar das atividades de lazer em Grupos de Terceira Idade representa a "saída do fundo de poço", traz um sentido para a vida e o próprio renascimento.

  14. Fatores relacionados à qualidade de vida de idosos em programas para a terceira idade

    Directory of Open Access Journals (Sweden)

    Nathaly Wehbe Dawalibi

    2014-08-01

    Full Text Available O envelhecimento populacional é um fenômeno social e requer atenção dos profissionais da saúde. O objetivo deste artigo foi analisar a influência de possíveis fatores intervenientes sobre a qualidade de vida de idosos.Trata-se de um estudo transversal, de natureza quantitativa, descritivo-exploratório, do qual participaram 182 idosos, de ambos os gêneros, ≥ 60 anos, matriculados em programas para a terceira idade de três universidades localizadas nos municípios de São Paulo, São Caetano do Sul e Mogi das Cruzes. Para avaliar a percepção subjetiva da qualidade de vida, utilizou-se o World Health Organization Quality of Life Questionnaire (WHOQOL-Bref. Foi realizada análise de regressão linear múltipla entre as variáveis dependentes e independentes. Adotou-se nível de significância de 5%. Os resultados mostraram que a ausência de doenças influenciou positivamente a qualidade de vida nos quatro domínios avaliados. No domínio ambiental, ensino superior completo, idade avançada, ausência de doenças e residência em São Caetano do Sul influenciaram positivamente a qualidade de vida dos idosos estudados. Os fatores associados à melhor qualidade de vida foram: ensino superior completo, idade avançada, ausência de doenças e residência em São Caetano do Sul, nessa ordem de importância.

  15. Nova Era: uma manifestação de fé da contemporaneidade

    Directory of Open Access Journals (Sweden)

    Fabiano Fernandes Serrano Birchal

    2009-05-01

    Full Text Available O homem contemporâneo vive um mundo de incertezas, onde muitos dos antigos paradigmas que o senso comum considerava como absolutos se desmoronam com incrível velocidade. Esta volatilidade de sentidos é observada com ampla nitidez na busca do sagrado: as religiões tradicionais são deixadas de lado ou misturadas a práticas esotéricas, místicas e ocultas, tentativa humana de explorar o mundo através de um enfoque holístico, que reimprima na vida a magia outrora perdida. Neste contexto de construção de uma nova realidade, a percepção e manifestação do sagrado não desaparecem, mas, seguindo a mentalidade de seu tempo, transformam-se. A religiosidade assume um caráter individualista, imediatista e descompromissado, restaurando conceitos e práticas da antigüidade, em uma tentativa clara de reencantamento do mundo, agora sob a perspectiva da sociedade globalizada. Filosofias orientais invadem a dimensão religiosa do mundo ocidental, numa mistura explicitamente paradoxal. Deste epicentro nasce a cultura da Nova Era, movimento que busca restaurar a tradição sagrada do homem postulando um saber místico, pretendendo conectar o ser humano ao transcendente partindo não de instituições específicas, mas de conhecimentos e práticas do esoterismo, ocultismo e magia.Palavras-chave: Nova Era; Subjetivismo; Consumismo.ABSTRACTContemporary man lives in a world of uncertainties, where many of the old paradigms that common sense used to consider absolute are falling apart with incredible speed. Such volatility of senses is clearly noticed in the search for the sacred: traditional religions are left behind or mingled with esoteric, mystical and occult practices, in a human attempt to explore the world from a holistic viewpoint capable of rescuing life’s lost magic. In that context of construction of a new reality, the perception and manifestation of the sacred do not disappear; they rather change, following the mentality of the times

  16. Anemia em idade geriátrica : uma revisão da literatura

    OpenAIRE

    Miranda, Emanuel Cardoso Marques de

    2014-01-01

    Anemia em idosos é muito comum e é atribuída incorrectamente ao normal envelhecimento, sendo na maioria das vezes uma condição modificável e, como tal, deve ser gerida de forma pró-activa. A prevalência de anemia aumenta com a idade e esta é muito maior entre os residentes em lares de idosos do que entre idosos residentes na comunidade. Nesta faixa etária, as causas de anemia são geralmente multifactoriais. Os indivíduos mais velhos com anemia, mesmo aqueles com níveis baixos ou no limiar ...

  17. Meningites em idade pediátrica – realidade de um hospital português

    OpenAIRE

    Silva, Rita Santos; Gonçalves, Daniel; Carvalho,Fernanda; Fonseca, Paula; Carvalho, Sónia; Teixeira, Paulo

    2013-01-01

    Objectivo: Descrever os doentes internados por meningite após o período neonatal.Material e métodos: Estudo retrospectivo, através da consulta dos processos clínicos dos doentes internados por meningite num hospital nível II do Norte de Portugal entre Janeiro de 2002 e Julho 2010.Resultados: A amostra incluiu 89 doentes, 75% do sexo masculino, com mediana de idades de 3 anos (1 mês-14 anos). Ocorreram onze casos (12%) de meningites bacterianas, 29 (33%) víricas, 11 (12%) parcialmente tratadas...

  18. Planejamento familiar: significado para mulheres em idade reprodutiva Family planning: significance for women of reproductive age

    OpenAIRE

    Raimunda Magalhães da Silva; Kelly Nóbrega Cavalcante de Araújo; Lya Araújo Costa Bastos; Escolástica Rejane Ferreira Moura

    2011-01-01

    O estudo teve como objetivo compreender o significado do planejamento familiar dado por mulheres em idade reprodutiva, identificar suas percepções sobre a assistência recebida e a participação do parceiro nas decisões do uso do método anticoncepcional. Trata-se de um estudo descritivo, com abordagem qualitativa, desenvolvido com 24 mulheres que participavam do Programa de Planejamento Familiar (PF) em uma Unidade Básica de Saúde da Família de Fortaleza (Ceará), no período de agosto a outubro ...

  19. Exigência de triptofano para frangos de corte de 1 a 21 dias de idade

    OpenAIRE

    Castro Altivo José de; Gomes Paulo Cezar; Pupa Júlio Maria Ribeiro; Rostagno Horacio Santiago; Albino Luiz Fernando Teixeira; Nascimento Adriana Helena

    2000-01-01

    Com o objetivo de determinar as exigências nutricionais em triptofano para frangos de corte machos e fêmeas, durante a fase inicial, foram utilizados 800 pintos machos e fêmeas, no período de 1 a 21 dias de idade, com peso médio inicial de 44,7 e 44,6 g, respectivamente. As aves receberam uma dieta basal deficiente em triptofano (0,180%). O delineamento experimental utilizado foi em blocos casualizados em arranjo fatorial 5 x 2 (tratamento x sexo), com quatro repetições por sexo e 20 aves/uni...

  20. Comportamento de lactentes nascidos a termo pequenos para a idade gestacional no primeiro trimestre da vida

    OpenAIRE

    2004-01-01

    O objetivo foi comparar o comportamento de lactentes nascidos a termo com peso adequado (AIG) a lactantes pequenos para a idade gestacional (PIG), no primeiro trimestre de vida. A amostra foi de 20 lactentes, avaliados no 1º, 2º e 3º meses. Foram utilizadas as Escalas Bayley de Desenvolvimento Infantil - II, com ênfase na Escala de Classificação do Comportamento (ECC). Houve diferença significativa entre os grupos no 2º mês, com maior número de lactentes PIG classificados como alterados na EC...

  1. Estimativa da estrutura em portugueses com idade igual ou superior a 60 anos

    OpenAIRE

    2009-01-01

    Dissertação de mestrado em Medicina (Geriatria), apresentada à Faculdade de Medicina da Universidade de Coimbra A desnutrição, sobretudo em idades geriátricas, é um factor de risco global e agrava um grande número de patologias. A medida do estado nutricional mais generalizada na actualidade é o Índice de Massa Corporal, para o qual se consideram as variáveis peso e estatura. Quando a estatura não pode ser medida correctamente, há dificuldade em determinar o IMC. A incapacid...

  2. 大兴安岭哈拉哈河-绰尔河第四纪火山分期:K-Ar年代学与火山地质特征%Studies on Quaternary volcanism stages of Halaha river and Chaoer river area in the Great Xing'an Range: Evidence from K-Ar dating and volcanic geology features

    Institute of Scientific and Technical Information of China (English)

    樊祺诚; 赵勇伟; 李大明; 武颖; 隋建立; 郑德文

    2011-01-01

    34 Quaternary volcanoes are distributed along a Quaternary NE strike belt in Halaha river and Chaoer river volcanic field. The lava flow, characterized by alkali olivine basalts, cover an area of 400km2. Based on studies on the volcanic field characteristics, in conjunction with geological dating by K-Ar, it is identified that the volcanism occurred in four periods; Early Pleistocene, Middle Pleistocene, Late Pleistocene and Holocene. Basalts of Early Pleistocene, mostly mantled by the later volcanic rocks, are distributed in the margin and valleys of the volcanic field. Middle Pleistocene, the most volcanic active period in this area, witnessed the formation of more than half of Quaternary volcanoes and lava spreading. Moderate volcanism occurred in Late Pleistocene which produced a small amount of volcanic deposits. Volcanic activities are strengthened again in Holocene Period, characterized by strongly explosive explosion, widespread lava flow and well-keeping lava landforms features.%大兴安岭中部哈拉哈河-绰尔河第四纪火山区分布有34座火山,这些火山总体呈北东向带状分布,火山岩分布面积约400 km2,岩性主要为碱性橄榄玄武岩.根据火山地质特征,结合火山岩K-Ar测年结果,哈拉哈河-绰尔河第四纪火山可进一步划分为早、中、晚更新世和全新世4期.早更新世火山岩,由于被后期火山岩覆盖,主要分布于火山区周边和出露在河谷中.中更新世火山活动最强,不论火山数量(27座)还是熔岩流规模都超过该区第四纪火山的一半以上.晚更新世时期火山活动趋弱,火山活动范围缩小,只局限于小范围区域.全新世火山活动又进入新的高峰期,强爆破式喷发和规模宏大的熔岩流,以及保存完好的熔岩流地貌是全新世火山之特点.

  3. 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

  4. 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.

  5. 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.

  6. 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.

  7. 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

  8. 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.

  9. 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.

  10. 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...

  11. 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...

  12. 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

  13. 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

  14. 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)

  15. 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

  16. 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.

  17. 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.

  18. 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…

  19. 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.

  20. 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.

  1. 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.

  2. Desempenho motor de idosos do Nordeste brasileiro: diferenças entre idade e sexo

    Directory of Open Access Journals (Sweden)

    Paloma Andrade Pinheiro

    2013-02-01

    Full Text Available O objetivo deste estudo foi identificar o desempenho motor, de acordo com o sexo e o grupo etário, em idosos residentes em comunidade do Nordeste brasileiro. Trata-se de estudo transversal que analisou dados de 316 idosos de uma pesquisa epidemiológica de base domiciliar e populacional realizada em janeiro de 2011. Participaram do estudo 173 mulheres (54,7% e 143 homens com idade média de 74,2 (± 9,8 anos. As mulheres apresentaram maior declínio funcional com o avanço da idade e mais limitação funcional em testes de força/resistência de membros inferiores e locomoção. Em ambos os sexos, a prevalência de limitação funcional foi mais elevada nos grupos etários de 70-79 anos e > 80 anos, com as mulheres apresentando mais limitação a partir dos 70 anos e os homens, a partir dos 80 anos. Os dados desta pesquisa podem subsidiar o planejamento de medidas para prevenção, manutenção ou melhora da limitação funcional em idosos, proporcionando maiores cuidados integrados.

  3. Morfologia e Crescimento dos 6 aos 10 anos de idade em Viana do Castelo, Portugal

    Directory of Open Access Journals (Sweden)

    Luis Paulo Rodrigues

    2008-09-01

    Full Text Available Ao longo de quatro anos, o Estudo Morfofuncional da Criança Vianense observou 1911 crianças entre os 6e os 10 anos de idade, resultando em 4064 observações individuais(2054 de raparigas, 2006 de rapazes.Os resultados encontrados nos indicadores morfológicos simples(altura, peso, pregas adiposas, diâmetros ósseos e perímetros muscularese no somatótipo, são descritos normativamente (valores percentílicose comparados com outros estudos nacionais e internacionais. As crianças vianenses demonstraram possuir uma estatura média ligeiramente superior às reportadas nos estudos portugueses e um ritmo de crescimento diferente das norte-americanas; peso semelhante ao das congéneres nacionais mas inferior ao das EUA; valores de pregas adiposas geralmente inferiores aos encontrados em Portugal e EUA; perímetros musculares e diâmetros ósseos semelhantes aos seus pares portugueses; e uma tendência para o aumento, com a idade, do ectomorfismo nos rapazes e do endomorfismo em ambos os sexos. Este panorama parece indicar que as crianças vianenses apresentam características de aptidão morfologia que estão longe de espelhar as preocupações internacionais nesta matéria.

  4. 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...

  5. 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...

  6. 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)

  7. 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)

  8. 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...

  9. Estimativa da prevalência de déficit de altura/idade a partir da prevalência de déficit de peso/idade em crianças brasileiras

    Directory of Open Access Journals (Sweden)

    Victora Cesar G.

    1998-01-01

    Full Text Available INTRODUÇÃO: A antropometria é amplamente utilizada para avaliação nutricional de indivíduos e de grupos populacionais. Em anos recentes, diagnósticos comunitários têm sido realizados por profissionais dos serviços de saúde em diversas regiões brasileiras, com o objetivo de complementar os dados obtidos através de vigilância nutricional. Um obstáculo importante à realização destes diagnósticos é a difícil mensuração da altura em inquéritos domiciliares. MÉTODO: Foram identificados 38 inquéritos antropométricos com crianças de 0 a 5 anos de idade, realizados no Brasil, que utilizaram o padrão de referência NCHS e o percentual de crianças abaixo de -2 escore Z para definição da prevalência de déficit de peso/idade e altura/idade. A análise foi realizada a partir das correlações entre as prevalências de déficits de altura/idade e peso/idade definidas. RESULTADOS: A análise mostrou que devido à baixa prevalência de déficits de peso/altura há forte correlação entre peso/idade e altura/idade, em nível populacional. Cerca de 90% da variabilidade de altura/idade (A/I é explicada pelo peso/idade (P/I. CONCLUSÃO: Através da equação (Prev. A/I = 0,74 + 2,34 (Prev. P/I - 0,03 (Prev. P/I2, é possível estimar os déficits de altura, desde que se conheça os déficits de peso. Espera-se que os resultados possam contribuir para a simplificação dos inquéritos antropométricos realizados no âmbito dos serviços e favorecer sua disseminação.

  10. 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 ...

  11. IDADE DA PRIMEIRA CRIA EM GADO NELORE AGE AT FIRST CALVING IN NELORE CATTLE

    Directory of Open Access Journals (Sweden)

    José Magno Pato

    2007-09-01

    Full Text Available

    O presente estudo de 118 dados de idade à primeira cria de criação de Nelore da Fazenda Regional de Criação do Ministério da Agricultura, Goiânia - Goiás, mostrou uma média 50,49 +/- 0,90 meses.

    The present study of 118 data of first calving age in Nelore cattle of the Fazenda Regional de Criação do Ministério da Agricultura, Goiânia—Goiás, showed an average of 50.49 +/- 0.90 months.

  12. Aspectos psicossociais e qualidade de vida da degenerescência macular relacionada com a idade

    OpenAIRE

    Silva, I; José Pais Ribeiro

    2006-01-01

    A degenerescência macular relacionada com a idade é uma patologia que provoca diminuição da acuidade visual e possível perda irreversível da visão, constituindo a principal causa de cegueira nos países ocidentais. Trata-se de uma doença crónica com tendência aumentar e que tem um significativo impacto na vida do doente e da sua família, bem como um impacto colossal em termos económicos para os sistemas de saúde, o que tem contribuído para o interesse crescente pelo desenvolvime...

  13. Tempos de aprender: a produção histórica da idade escolar

    Directory of Open Access Journals (Sweden)

    Maria Cristina Soares de Gouveia

    2012-02-01

    Full Text Available A emergência de um tempo escolar, nas sociedades ocidentais, com o advento da Modernidade, relaciona-se com a definição de um marco cronológico no decorrer da vida do indivíduo, ao longo do qual este deveria inserir-se na escola, a chamada idade escolar. Esse marco constitui não um recorte absoluto, mas é fruto de uma construção histórica, ao longo da qual se modificaram os parâmetros de sua definição. Para analisar essa relação, cabe compreender a produção da representação da infância como período de formação para a vida adulta, no interior da instituição escolar, de acordo com princípios pedagógicos característicos de tal instituição. Princípios esses centrados no pressuposto da educabilidade desse período de vida. Tal pressusposto tornou possível a emergência, no decorrer do século XIX, em diferentes países, das leis de obrigatoriedade escolar, que conferiram visibilidade social à idade da meninice (por volta dos 7 aos 14 anos entendida como idade escolar. Tendo como fontes primárias a legislação educacional e a documentação referente à instrução pública, busca-se analisar, no contexto da província mineira, o significado da noção de idade escolar ao longo do período e suas características, de modo que se apreendam suas permanências e deslocamentos. Abstract The emergence of a “scholar time” in occidental societies in modernity is related with the historical conformation process of an “scholar age”. In this sense, its necessary to understand the construction of childhood as the period of life when the individuate must be prepared to adult society, according to pedagogical principles in a school institution.Those principles are centred on the idea of childhood specificity, there educability. That notion turned possible the school, and the emergence of the “obligation scholar laws”, in differents nations, during the nineteen century, that institucionalized a scollar time into social

  14. Reações de hipersensibilidade a meios de contraste em idade pediátrica

    OpenAIRE

    Almiro, Maria Miguel; Maia, Catarina; Branco, Liliana; Pedrosa, Cláudia; Romariz, Jorge; Praça, Fátima; Costa, Herculano

    2016-01-01

    Introdução: Os procedimentos diagnósticos e terapêuticos com utilização de produtos de contraste são muito frequentes na prática clínica. Qualquer um destes agentes pode ser responsável por reações de hipersensibilidade, com um amplo espetro de gravidade. Objetivos: Revisão da epidemiologia, manifestações clínicas, diagnóstico e prevenção das reações de hipersensibilidade aos produtos de contraste em idade pediátrica. Desenvolvimento: Os produtos de contraste incluem meios radiológico...

  15. Hipersensibilidade medicamentosa em crianças de idade pré-escolar

    OpenAIRE

    Jorge Da Costa Viana; Carmo Abreu; Eva Rebelo Gomes

    2016-01-01

    Introdução: As reações de hipersensibilidade medicamentosa (RHM) são reacções adversas reprodutíveis que se caracterizam por sintomas típicos de alergia que surgem após administração de doses terapêuticas habituais. A sua prevalência em idade pediátrica atinge os 10%. A investigação das RHM inclui a realização de testes cutâneos, pesquisa de imunoglobulinas específicas para os alergénios implicados e provas de provocação. Objectivos: No presente trabalho pretendemos relatar os resultados d...

  16. Hipersensibilidade medicamentosa em crianças de idade pré-escolar

    OpenAIRE

    Viana, Jorge da Costa; Abreu, Carmo; Gomes, Eva Rebelo

    2016-01-01

    Introdução: As reações de hipersensibilidade medicamentosa (RHM) são reacções adversas reprodutíveis que se caracterizam por sintomas típicos de alergia que surgem após administração de doses terapêuticas habituais. A sua prevalência em idade pediátrica atinge os 10%. A investigação das RHM inclui a realização de testes cutâneos, pesquisa de imunoglobulinas específicas para os alergénios implicados e provas de provocação.Objectivos: No presente trabalho pretendemos relatar os resultados da in...

  17. OS ASPECTOS ÉTICOS QUE ENVOLVEM A EDUCAÇÃO NA TERCEIRA IDADE

    Directory of Open Access Journals (Sweden)

    Fábio Luiz Villani

    2010-01-01

    Full Text Available Durante muitos anos a educação de idosos foi considerada desnecessária em nossa sociedade, pois somente crianças e jovens adultos tinham o direito a esse privilégio em nossas escolas. Somente nos últimos anos, com o aumento da expectativa de vida, a sociedade começou a pensar e criar condições para um envelhecimento intelectualmente saudável por meio da educação continuada. Neste artigo, objetiva-se mostrar a necessidade de desenvolver um caminho na educação para melhorar a vida da comunidade da terceira idade. Como aspectos ligados à moral e à ética poderiam ajudar a mudar o ponto de vista da sociedade a respeito dessas pessoas? Palavras-chave: ética; educação; gerontologia.

  18. Um estudo das capacidades e deficiências em habilidades sociais na terceira idade

    Directory of Open Access Journals (Sweden)

    Carneiro Rachel Shimba

    2004-01-01

    Full Text Available Esta pesquisa pretende identificar as situações sociais nas quais os idosos apresentam facilidades e dificuldades de se comportar de forma socialmente habilidosa. Foram entrevistados 30 idosos da Universidade Aberta da Terceira Idade. A partir da análise dos dados pôde-se identificar um percentual maior de respostas habilidosas em seis situações sociais. Por outro lado, a maioria dos idosos da amostra apresentou deficiências de desempenho em oito situações sociais. Os resultados propõem o desenvolvimento de programas de treinamento de habilidades sociais como uma forma de aumentar a capacidade do idoso de conquistar e manter apoio social, para assim, alcançar melhor qualidade de vida.

  19. DANÇAS MACABRAS: UMA CRÍTICA SOCIAL NA BAIXA IDADE MÉDIA

    Directory of Open Access Journals (Sweden)

    José Carlos Gimenez

    2011-09-01

    Full Text Available Este artigo realiza uma reflexão sobre o significado da morte retratado nas manifestações culturais conhecidas como Danças Macabras ou Danças da Morte; um gênero alegórico muito difundido no final da Idade Média e início do período Renascentista e que tem por objetivo discutir a fragilidade do homem diante da presença inevitável da morte. A análise é feita a partir da leitura do texto anônimo Danza General de Muerte, escrito entre os séculos XIV e XV.

  20. 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.

  1. 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.

  2. 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.

  3. 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++.

  4. 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.

  5. 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.

  6. 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.

  7. 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.

  8. 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.

  9. 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.

  10. 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.

  11. 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.

  12. 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...

  13. 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.

  14. 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”).

  15. Qualidade de pintos em função do microclima, tempo de espera e idade de matrizes

    OpenAIRE

    Camargo,Juliano R. de; Iran J. O. da Silva; Nazareno,Aérica C.; Vieira,Frederico M. C.; Ariane C. de Castro; Dias,Raphael A. P.

    2015-01-01

    RESUMOPropôs-se avaliar a influência das condições microclimáticas do tempo de espera na sala de pintos do incubatório sobre a qualidade final dos pintos de um dia, oriundos de matrizes de diferentes idades. Foi mensurada a massa de 1440 ovos férteis, divididos em três lotes de 480 ovos cada um referentes às idades de matrizes (46, 54 e 64 semanas). Após o nascimento os pintos foram selecionados, sexados e subdivididos nas três idades de matrizes e em três tempos de espera (0, 14 e 28 h). Tam...

  16. 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...

  17. 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.

  18. 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.

  19. 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...

  20. 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

  1. 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...

  2. 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, ...

  3. 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...

  4. 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 ...

  5. 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...

  6. 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.

  7. 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...

  8. Correlação da massa e porcentagem de gordura com a idade na distrofia muscular de Duchenne

    OpenAIRE

    Caromano, Fátima Aparecida; Tanaka,Clarice; João,Sílvia Maria Amado; Kamisaki,Ana Patrícia; YANO, Kelly Cristina; Ide,Maiza Ritomy

    2010-01-01

    INTRODUÇÃO: A Distrofia Muscular de Duchenne (DMD) é uma desordem genética, caracterizada pela perda progressiva e irreversível da musculatura esquelética. OBJETIVO: Este estudo objetiva correlacionar a porcentagem e a massa de gordura com a idade em pacientes com DMD. METODOLOGIA: Foram selecionados 68 indivíduos com idades entre 5 e 20 anos, com diagnóstico molecular de certeza para DMD, residentes na cidade de São Paulo. Todos foram submetidos à mensuração do peso e altura e também ao test...

  9. 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.

  10. 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.

  11. 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.

  12. 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).

  13. 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.

  14. 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...

  15. 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.

  16. 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.

  17. Pequenos para idade gestacional: fator de risco para mortalidade neonatal Small for gestational age

    Directory of Open Access Journals (Sweden)

    Márcia Furquim de Almeida

    1998-06-01

    Full Text Available OBJETIVO: Estudar as variáveis contempladas na Declaração de Nascimento (DN como possíveis fatores de risco para nascimentos pequenos para a idade gestacional (PIG e o retardo de crescimento intra-uterino como fator de risco para a mortalidade neonatal. MATERIAL E MÉTODO: As variáveis existentes na DN foram obtidas diretamente de prontuários hospitalares. Os dados referem-se a uma coorte de nascimentos obtida por meio da vinculação das declarações de nascimento e óbito, correspondendo a 2.251 nascimentos vivos hospitalares, de mães residentes, ocorridos no Município de Santo André, Região Metropolitana de São Paulo, no período de l/1 a 30/6/1992, e aos óbitos neonatais verificados nessa coorte. RESULTADOS: Obteve-se a proporção de 4,3% de nascimentos PIG, significativamente maior entre os recém-nascidos de pré-termo e pós-termo, entre os nascimentos cujas mães tinham mais de 35 anos de idade e grau de instrução inferior ao primeiro grau completo. Os recém-nascidos PIG apresentam maior risco de morte neonatal que aqueles que não apresentavam sinais de retardo de crescimento intra-uterino. CONCLUSÕES: Em áreas com menor freqüência de baixo peso ao nascer, é importante investigar a presença de retardo de crescimento intra-uterino entre os nascimentos prematuros e não apenas nos nascimentos de termo. O registro da data da última menstruação (ou da idade gestacional em semanas não agregadas na DN facilitaria a detecção de PIGs na população de recém-nascidos.INTRODUCTION: Variables of birth certificates were analysed as risk factors of SGA (Small for Gestational Age infantis, and with a view to discovering if retarded intra-uterine growth was a risk factor neonatal mortality. MATERIAL AND METHOD: Data were obtained directly from 11 hospital medical records. A cohort of 2.251 hospital live births was obtained. Linkage of the death and birth certificates was undertaken to identify the neonatal deaths. The

  18. Escore CRIB, peso ao nascer e idade gestacional na avaliação do risco de mortalidade neonatal

    Directory of Open Access Journals (Sweden)

    Angela Sara J de Brito

    2003-10-01

    Full Text Available OBJETIVO: Avaliar a mortalidade dos recém-nascidos de muito baixo peso em uma UTI neonatal conforme as variações do escore CRIB (Clinical Risk Index for Babies, do peso de nascimento e da idade gestacional em determinado período. MÉTODOS: O escore CRIB foi aplicado seqüencial e prospectivamente em todos os recém-nascidos com peso de nascimento 10 (79,4%. A curva ROC (Receiver Operator Characteristic para os valores de CRIB, peso de nascimento e idade gestacional gerou áreas sob a curva de 0,88, 0,76 e 0,81, respectivamente. Na análise bivariada, o CRIB, peso e idade gestacional mostraram-se preditores de mortalidade, sendo o escore CRIB>4 o de melhor resultado com sensibilidade de 75,8%, especificidade de 86,7%, valor preditivo positivo de 63,3% e valor preditivo negativo de 92,2%. CONCLUSÕES: Os recém-nascidos com peso de nascimento 10 tiveram maiores taxas de mortalidade, sendo o escore CRIB>4 o que representou melhor poder preditivo quando comparado com peso ao nascer e idade gestacional.

  19. A proporción da escultura galaica na Idade do Ferro

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    Santos Estévez, Manuel

    2012-12-01

    Full Text Available This paper argues for the use of the so called Harmonic Proportion or Golden Proportion in a specific kind of Iberian Iron Age sculptures from southern Gallaecia. We suggest that the employment of such a sophisticated concept in the solution of a set of technical problems points at the existence of a specialized craftsman. We suggest that warrior sculptures were an instrument legitimating a ruling social group in the context of a complex chiefdom. These sculptures were used as ideological artefacts during Gallaecia’s Late Iron Age, and as a material representation of the social power.

    El artículo analiza el uso de la conocida como Proporción Armónica o Proporción Áurea en un tipo concreto de esculturas en el noroeste de la Iberia de la Edad del Hierro procedentes del sur de Gallaecia. Se propone que la aplicación de un concepto tan elaborado en la solución de una serie de problemas técnicos implica la existencia de artesanos especializados. Se considera que las esculturas de guerreros fueron un instrumento de legitimación de un grupo social dominante en un contexto de una sociedad de jefatura compleja. Estas esculturas, como artefactos ideológicos, fueron usadas en la Gallaecia de la tardía Edad del Hierro como una representación material del poder social. [gl] O artigo analiza o uso da coñecida como Proporción Harmónica ou Proporción Áurea nun tipo concreto de esculturas no noroeste da Iberia da Idade do Ferro procedentes do sur de Gallaecia. Proponse que a aplicación dun concepto tan elaborado na solución dunha serie de problemas técnicos implica a existencia de artesáns especializados. Considérase que as esculturas de guerreiros foron un instrumento de lexitimación dun grupo social dominante nun contexto dunha sociedade de xefatura complexa. Estas esculturas, como artefactos ideolóxicos, foron usadas na Gallaecia da tardía Idade do Ferro como unha representación material do poder social.

  20. Efeitos da idade da matriz leve e do período de armazenamento de ovos incubáveis no rendimento de incubação Effects of ages of light breeder hens and storage period of hatchable eggs on the incubation efficiency

    Directory of Open Access Journals (Sweden)

    C.B.G.S. Tanure

    2009-12-01

    Full Text Available Avaliaram-se os efeitos da idade das matrizes leves e do período de armazenamento dos ovos sobre o rendimento de incubação. Foram utilizados 7.224 ovos da linhagem Dekalb, distribuídos de acordo com delineamento experimental inteiramente casualizado, sendo a altura de bandeja uma covariável. Os tratamentos foram definidos pelas idades das matrizes (32 e 57 semanas de idade e o período de armazenamento dos ovos (três, cinco e sete dias, totalizando seis tratamentos com 14 repetições. A idade das aves influenciou o peso do ovo. Houve aumento na perda de peso dos ovos das matrizes de 32 e 57 semanas de idade, durante o armazenamento (10,48 e 14,16%, respectivamente e na transferência (10,40 e 12,07%, respectivamente. Verificou-se maior taxa de eclosão (86,90% em ovos produzidos pelas matrizes novas. Independentemente da idade da matriz, à medida que aumentou o período de armazenamento, houve diminuição na taxa de eclosão dos ovos férteis (86,06 e 82,39%, para as matrizes de 32 e 57 semanas de idade, respectivamente. As matrizes com 57 semanas de idade produziram pintos mais pesados e com menor relação peso do pinto/peso do ovo.The effects of ages of light breeder hens and storage period of hatchabe eggs on the incubation efficiency were evaluated. A total of 7,224 Dekalb hatching eggs were assigned according to the sample random design, and the hatching tray height was considered a co-variable. The treatments were defined according to the breeder hens ages (32 and 57-week-old and the period of storage of eggs (three, five, and seven days, with 14 replications. The age of the hen affected the weight of the eggs. There was loss of weight of the eggs of 32 and 57-week-old breeder hens during storage (10.48 and 14.16%, respectively and transference (10.40 and 12.07%, respectively according to the aging of the breeder hen. Eggs produced by the younger breeder hens had a higher hatching rate; however, no matter the age of the breeder

  1. 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

  2. Bipolar disorder and age-related functional impairment Prejuízo funcional associado à idade e transtorno bipolar

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    Alice Aita Cacilhas

    2009-12-01

    Full Text Available OBJECTIVE: Although bipolar disorder is a major contributor to functional impairment worldwide, an independent impact of bipolar disorder and ageing on functioning has yet to be demonstrated. The objective of the present study was to evaluate the effect of bipolar disorder on age-related functional status using matched controls as a standard. METHOD: One-hundred patients with bipolar disorder and matched controls were evaluated for disability. Age-related effects controlled for confounders were cross-sectionally evaluated. RESULTS: Patients were significantly more impaired than controls. Regression showed effects for aging in both groups. The effect, size, however, was significantly stronger in patients. CONCLUSION: Bipolar disorder was an important effect modifier of the age impact on functioning. While a longitudinal design is needed to effectively demonstrate this different impact, this study further depicts bipolar disorder as a chronic and progressively impairing illness.OBJETIVO: O transtorno bipolar é responsável por importante parcela do prejuízo funcional ao redor do mundo. Um efeito independente do transtorno bipolar e da idade no funcionamento ainda não foi demonstrado. O presente estudo tem o objetivo de avaliar o efeito do transtorno bipolar no prejuízo funcional relacionado à idade, com controles pareados como padrão. MÉTODO: Cem pacientes com transtorno bipolar e controles pareados foram avaliados para incapacidade. Efeitos relacionados à idade, com controle para confundidores, foram investigados. RESULTADOS: Pacientes tiveram significativamente mais prejuízo que controles. A regressão mostrou efeito para a idade em ambos os grupos, e o efeito foi significativamente mais forte nos pacientes. CONCLUSÃO: O transtorno bipolar foi um importante modificador de efeito no impacto da idade no funcionamento. Enquanto um desenho de estudo longitudinal é necessário para efetivamente demonstrar este impacto diferencial, este

  3. Influência da idade dos pais em recém-nascidos portadores da Síndrome de Down

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    Júlio Boschini Filho

    2007-05-01

    Full Text Available Nesta pesquisa, investigamos mediante estudo retrospectivo, a influência da idade dos pais nos recém-nascidos portadores da síndrome de Down, diagnosticados clínica e citogeneticamente no Serviço de Genética Clínica do Conjunto Hospitalar de Sorocaba (CHS nos últimos vinte anos. As análises cromossômicas foram realizadas em 50 metáfases de linfócitos com coloração convencional de Giemsa e bandamento G em 85 recém-nascidos masculinos e 63 femininos portadores da síndrome de Down. Os resultados revelam que a idade média paterna se apresentou maior entre os recém-nascidos masculinos (36 anos quando comparada aos femininos (33 anos; a diferença, porém, não foi significante. Quanto à variação (idade do pai – idade da mãe, verificamos que é significantemente maior entre os recém-nascidos masculinos (4,2 anos quando comparada a dos femininos (2,2 anos. Portanto, esta nossa pesquisa é indicativa de que a idade paterna tem influência nos eventos cromossômicos durante a gametogênese, principalmente na segregação dos cromossomos 21 e Y, implicados na ocorrência e predominância do sexo masculino entre os recém-nascidos com síndrome de Down.

  4. 大兴安岭诺敏河第四纪火山岩分期:岩石学、年代学与火山地质特征%Studies on Quaternary volcanism stages of Nuomin river area in the Great Xing'an Range: Evidence from petrology, K-Ar dating and volcanic geology features

    Institute of Scientific and Technical Information of China (English)

    樊祺诚; 赵勇伟; 隋建立; 李大明; 武颖

    2012-01-01

    大兴安岭北段诺教河第四纪火山24座,分布于诺敏河及其支流毕拉河和甘河支流奎勒河,火山岩分布面积约600km2.诺敏河火山岩均属于钾质系列火山岩(K2O含量2%~4%,且K2O> Na2o-2%),类似于邻区五大连池-科洛钾质火山岩,具有来自类似的富钾地幔源区.但诺敏河火山岩的K2O含量明显低于五大连池-科洛火山岩的K2O含量(一般4%~6%).东北地区和内蒙东部处于中亚造山带东段,从古生代到新生代,多重构造-岩浆活动导致火山岩源区地球化学非均一性和火山岩的多样性.根据本文提出的火山岩K-Ar年龄(2.3 ~0.128Ma)及火山地质特征,可将诺敏河第四纪火山岩分为四期.早期(早更新世)火山活动主要沿诺敏河和奎勒河流域分布,火山产物多被晚期沉积物或火山产物所覆盖.中更新世保留的火山锥体及熔岩流是诺敏河第四纪火山产物的主体,表明是第四纪火山活动的高潮期.晚更新世-全新世火山活动限于毕拉河流域,典型的四方山火山和马鞍山火山是该时期火山活动的代表作,保留了较完好的火山地质地貌特征.从火山产物的时空展布,推测诺敏河第四纪火山活动有从东向西发展的趋势.%24 Quaternary volcanoes are distributed along IVnomin river and Kuile river area volcanic field ( NK for short) in the north of the Great Xing' an Range. With an area of 600 square kilometers, the volcanic rocks are characterized by potassic series (K2O =2% -4% , K2O > Na2O -2% ), which are similar with rocks in Wudalianchi-Keluo volcanic field (WK for short). Although NK and WK share the alike mantle source, volcanic rocks from NK are low in K2O than that from WK ( K2O = 4% ~6% ). During the Paleozoic and the Cenozoic, multiple tectonic and magmatic activities resulted in the heterogenous geochemistry in the magma source, and thus varied volcanic rocks were generated. Based on K-Ar dating (2.3 ~ 0. 128Ma) and

  5. Trombose venosa profunda em idade pediátrica – estudo retrospetivo de 10 anos

    Directory of Open Access Journals (Sweden)

    Ana Isabel Sequeira

    2016-09-01

    Discussão e Conclusão: A TVP na criança tem sido reconhecida como uma patologia rara, mas importante causa de morbilidade. A maior incidência de TVP foi documentada na adolescência com compromisso do membro inferior, tal como referido na literatura. Verificamos uma conjugação de fatores de risco que, provavelmente, se potenciaram entre si levando à ocorrência do TEV e colocamos a possibilidade do Pediatra se estar a deparar com uma nova realidade anteriormente excluída do atendimento pediátrico. O aumento na incidência desta patologia levanta a questão do acréscimo de risco trombótico nos adolescentes do sexo feminino devido à utilização de contracetivos orais combinados. Salientamos a importância de um consenso nacional no diagnóstico, tratamento e prevenção desta entidade em Pediatria.

  6. Idade: A manifestação de Cronos nos jornais paulistanos

    Directory of Open Access Journals (Sweden)

    Maria Helena Villas Bôas Concone

    2010-02-01

    Full Text Available A leitura dos recortes de jornais analisados nos trouxe à lembrança o pequeno livro O Papalagui. O livrinho traz as muitas reflexões de Tuiávii, dentre as quais aquelas sobre o modo pelo qual o “branco” (o Papalagui lida com o tempo. Os comentários do chefe de Tiavéa acusam a preocupação “ocidental” com o tempo, como uma espécie de compulsão e de urgência, quando não de loucura: o tempo é dividido, demarcado, contado, reificado, usado; de fato, Tuiávii faz uma distinção entre o usufruir do tempo e o usar o tempo num sentido utilitário. Palavras-chave: Tempo; Cronos; Jornais paulistas; Idade Age: The manifestation of Chronos in Sao Paulo newspapers ABSTRACT: The reading of newspaper clippings analyzed brought to our mind the small book The Papalagui. The book includes the many reflections of Tuiavii, among which there are those on the way in which the “white” (the Papalagui deals with time. The comments from the Tiavea chief accuse “western” concern with time as a kind of compulsion and urgency, if not madness: the time is divided, marked, counted, objectified, used actually. Tuiavii distinguishes between enjoying time and using time in a utilitarian sense. Keywords: Time; Chronos; Sao Paulo newspapers; Age

  7. Teor de metionina + cistina para codornas de corte do nascimento aos 21 dias de idade

    Directory of Open Access Journals (Sweden)

    T.Z.B. Vidal

    2015-02-01

    Full Text Available Estudou-se o efeito do teor de metionina + cistina sobre o desempenho de codornas de corte durante a fase inicial (nascimento ao 21° dia. Foram utilizadas 360 codornas, de ambos os sexos, distribuídas em delineamento experimental inteiramente ao acaso. Os tratamentos consistiram em seis níveis de metionina + cistina total (0,86; 0,96; 1,06; 1,16; 1,26 e 1,36, quatro repetições e 15 aves por unidade experimental. As características avaliadas foram o peso corporal, ganho de peso, consumo e conversão alimentar para fase inicial. Observou-se efeito quadrático significativo do teor de metionina + cistina sobre todas as variáveis avaliadas do nascimento ao 21° dia de idade, sendo observado melhor desempenho nas codornas alimentadas com 1,21% de metionina + cistina para peso corporal e ganho de peso, 1,36% de metionina + cistina para consumo e 1,1% de metionina + cistina para conversão alimentar. A exigência de metionina + cistina para máximo ganho de peso na fase inicial é de 1,21%.

  8. Macroprolactinoma aos 6 anos de idade dificuldades diagnósticas: difficulties in diagnosis

    Directory of Open Access Journals (Sweden)

    Miriam Da Costa Oliveira

    1992-09-01

    Full Text Available Prolactinoma é raro na infância e adolescência. O diagnóstico mais precoce conhecido na literatura ocorreu aos 8 anos de idade. Aqui é relatado o achado de tumor selar em menina com 6 anos, embora só fosse procurado auxílio médico tardiamente, quando a paciente já apresentava atrofia parcial de papila. Nessa ocasião, foi constatada reserva diminuída de hormônio do crescimento e de cortisol, bem como hiperprolactinemia. Devido à rápida deterioração visual, a paciente foi submetida a craniotomia fronto-temporal com a hipótese diagnóstica de craniofaringioma. O exame imuno-histoquímico do tecido tumoral foi positivo para prolactina. Conclui-se que o prolactinoma deve ser considerado no diagnóstico diferencial de tumores selares na infância, por possibilitar terapêutica menos agressiva.

  9. LITÍASE BILIAR EM IDADE PEDIÁTRICA – QUE ABORDAGEM?

    Directory of Open Access Journals (Sweden)

    Sara Leite

    2016-07-01

    Comentários: Neste caso, tal como referido na literatura, a presença de colelitíase comportou um risco acrescido de colédo- co-litíase sintomática. Contudo, a abordagem terapêutica não é consensual. Se por um lado na criança pequena a abordagem da litíase vesicular assenta numa atitude expectante, na presença de litíase biliar obstrutiva a terapêutica médica não é eficaz e a CPRE é o método terapêutico gold standard, mas a experiência em idade pediátrica é limitada. Neste caso, a ausência de ex- periência na realização de CPRE, nesta faixa etária, nas zonas Norte e Centro do país determinou que o procedimento se tenha realizado num Hospital de Lisboa.

  10. Os efeitos da idade na seleção de carga perceptual

    Directory of Open Access Journals (Sweden)

    Vanessa Coelho de Sousa

    Full Text Available Algumas pesquisas sugerem a existência de momentos distintos de maturação do sistema atentivo. O presente estudo investigou os padrões de seleção da informação visual através de uma tarefa de carga perceptual executada por três grupos etários: crianças, adultos e idosos. De maneira geral os resultados obtidos indicaram uma diminuição da eficiência no processo de seleção da informação em condições de baixa carga perceptual na população de idosos e uma diminuição da eficiência da seleção em condições de alta e baixa carga perceptual na população composta por crianças. Estes resultados sugerem a existência de padrões específicos na seleção da informação visual em função da idade e da carga perceptual a ser processada pelo sistema visual.

  11. 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.

  12. 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.

  13. 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.

  14. 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.

  15. 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.

  16. 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.

  17. 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...

  18. 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.

  19. 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...

  20. 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...

  1. 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...

  2. 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.

  3. 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...

  4. 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...

  5. 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.

  6. 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.

  7. 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.

  8. 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...

  9. 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.

  10. 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…

  11. 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,...

  12. Efeito da idade de abate no valor nutritivo e sensorial da carne caprina de animais mestiços

    Directory of Open Access Journals (Sweden)

    MADRUGA M. S.

    1999-01-01

    Full Text Available O efeito da idade de abate na composição centesimal e mineral, no pH, na atividade de água e nas qualidades sensoriais da carne caprina foi estudado, utilizando-se para tanto animais machos abatidos ao completarem 175, 220, 265 e 310 dias de nascimento. Após o abate e a desossa, a carne caprina foi submetida às análises físico-químicas de pH, Aw, Ca, Fe e P; às determinações de composição centesimal (umidade, cinzas, proteínas e gorduras e à análise sensorial, onde foram observados os atributos de: aparência, aroma "caprino", aroma de carne assada, sabor, suculência, maciez, textura e a qualidade da carne. A análise de Variância (ANOVA dos dados mostrou que as concentrações de umidade, proteínas, cálcio, ferro e pH foram significativamente influenciadas pelo fator idade de abate. Os teores de gordura, proteína e ferro aumentaram com a idade de abate, enquanto que a umidade diminuiu. Através dos teste da análise sensorial, ficou evidente que a idade dos caprinos apresentou um efeito significativo nos atributos sensoriais analisados, tendo-se detectado diferenças significativas entre os caprinos de diferentes idades de abate nos atributos de aparência, aroma "caprino", aroma de carne assada, suculência e maciez. A partir dos resultados das análises físico-químicas e sensoriais pôde-se observar, que o abate de animais mais velhos, isto é, com 310 dias, resultou em ganho nos parâmetros químicos (composição centesimal e mineral investigados, embora a carne de caprinos abatidos com menor idade (175 dias tivesse a preferência dos provadores.

  13. Análise química do bambu-gigante (Dendrocalamus giganteus Wall. ex Munro em diferentes idades

    Directory of Open Access Journals (Sweden)

    Nelson Potenciano Marinho

    2012-06-01

    Full Text Available http://dx.doi.org/10.5902/198050985749O bambu é uma planta monocotiledônea de origem tropical, de rápido crescimento, sendo considerado um importante regenerador ambiental devido ao seu sistema radicular. O Dendrocalamus giganteus é popularmente conhecido por bambu-gigante, sendo uma espécie entouceirante de grande porte, cujos colmos podem variar de 24 a 40 metros de altura, com diâmetros entre 10 e 20 cm. Esse trabalho teve como objetivo analisar quimicamente os colmos do bambu-gigante visando fornecer informações sobre a sua composição química nas idades de 2 a 6 anos. Os colmos do bambu foram coletados na área Experimental Agrícola do Departamento de Engenharia Mecânica da UNESP-Bauru, onde é realizado o manejo sistemático de diversas espécies de bambu para fins de pesquisas e divulgação dessa planta. Foram retiradas amostras da base entre bambus com idade de 2 a 6 anos de uma mesma touceira, totalizando 5 amostras, com 2 metros de altura cada, colhidas na lua minguante no mês de março. As análises químicas foram feitas com os entrenós, utilizando as normas e procedimentos da TAPPI. A porcentagem média de extrativos em água quente, extrativos em água fria, extrativos totais e teor de cinzas não apresentaram relação direta com a idade. A maior porcentagem de extrativos em água quente, com valor de 12,04%, extrativos em água fria, com 10,25%, e extrativos totais, com 12,91%, foi observada aos 2 anos de idade. A maior porcentagem de cinzas foi obtida aos três anos, com valores de 1,09%. O teor médio de extrativos em NaOH diminui de 25,72% aos dois anos para 20,17% aos seis anos de idade. O mesmo comportamento foi observado para os extrativos em etanol tolueno, diminuindo de 10,91% para 4,61%. O teor médio de lignina não sofreu influência da idade, variando de 22,66 a 24,11%.

  14. 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.

  15. 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...

  16. 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...

  17. 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...

  18. 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 ...

  19. 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...

  20. 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.

  1. 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.

  2. Optical spectroscopy of the dwarf nova U Geminorum

    CERN Document Server

    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...

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

    CERN Document Server

    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 ...

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

    Directory of Open Access Journals (Sweden)

    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.

  5. 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.

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

    CERN Document Server

    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.

  7. Eqüidade e reformas na saúde nos anos 90

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    Cohn Amélia

    2002-01-01

    Full Text Available O presente artigo analisa na primeira seção questões atuais colocadas para a agenda de estudos e debates sobre a Reforma Sanitária Brasileira da perspectiva da inclusão e da exclusão sociais. E numa segunda seção, à luz daquelas questões inicialmente discutidas, analisa uma experiência de parceria entre o setor público estatal (o Hospital das Clínicas ­ HC, Faculdade de Medicina, Universidade de São Paulo e o Sistema Supletivo de Assistência Médica (SSAM. A tese apresentada é a do esgotamento do ideário original da Reforma Sanitária Brasileira, após a conquista do movimento consagrado na Constituição de 1988, e frente à nova realidade do país, com a conseqüente necessidade de se resgatar a ênfase na dimensão política nos estudos sobre saúde, colocando em destaque a questão da construção de identidades dos sujeitos sociais. A partir dela é analisada a experiência daquela parceria, mostrando como a existência da "dupla fila" ­ a dos usuários SUS e a dos usuários do SSAM ­ não implica discriminações no acesso à tecnologia, mas reproduz no interior do HC as discriminações já existentes na sociedade.

  8. Aprendendo sobre eventos físicos com parceiros de idade

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    Maria Isabel Patrício de Carvalho Pedrosa

    2009-09-01

    Full Text Available Estudando crianças de 19 a 31 meses, numa perspectiva sociointeracionista, exploram-se diferentes situações de brincadeira com o parceiro de idade que parecem instigar aquisições e aprendizagens. O brincar é concebido como um espaço privilegiado de observação pelo valor motivacional prevalente que tem para as crianças. Por meio da brincadeira, ou mesmo para brincar, a criança lança mão de diversas estratégias na tentativa de resolver seus problemas (introduzir-se em um arranjo social já configurado, dirimir um conflito; chamar a atenção do parceiro, tecer o enredo do episódio, conseguir um resultado semelhante com o mesmo objeto etc.. Com este trabalho pretendeu-se evidenciar a potencialidade de diversos caminhos de aprendizagem sobre eventos físicos quando as crianças lidam com objetos deixados à sua disposição. Nos episódios selecionados para análise foi possível identificar quatro dinâmicas interacionais que revelam estratégias utilizadas pelas crianças em ações cooperativas que podem conduzir a aprendizagens e evidenciam que, mesmo bem pequenas, elas refletem sobre suas próprias ações e as de seus parceiros. Discutem-se algumas implicações teóricas e educacionais dessas evidências.

  9. Transtorno de personalidade na terceira idade Personality disorders in an elderly patient

    Directory of Open Access Journals (Sweden)

    Fernanda Speggiorin Pereira

    2007-01-01

    Full Text Available CONTEXTO: Dificuldades interpessoais, instabilidade afetiva, distorções da relação médico-paciente e respostas imprevisíveis às intervenções são características centrais aos transtornos de personalidade que são encontradas tanto em pacientes jovens, como em adultos idosos. RELATO DE CASO: Encontra-se aqui descrito um caso de transtorno de personalidade em paciente de 68 anos de idade, com transtorno de personalidade do tipo histriônica e outras comorbidades psiquiátricas. CONCLUSÃO: Transtorno de personalidade é um diagnóstico raramente aventado no tratamento psiquiátrico no paciente idoso de difícil manejo. Deve-se nestes casos fazer uma investigação mais aprofundada do funcionamento da personalidade, pois a presença e a severidade do transtorno de personalidade têm implicações no plano da assistência de ambos os tratamentos psicológico e farmacológico.CONTEXT: Interpersonal difficulties, affective instability, distortions of the clinician-patient relationship, and unpredictable responses to clinical interventions, are characteristics found in older adults as well as in younger patients with personality disorders. CASE REPORT: We report the case of a 68 years old patient with histrionic personality disorder and other psychiatric comorbidities. CONCLUSION: Personality disorders are frequently overlooked in the diagnostic workout of complex psychogeriatric syndromes, and require a comprehensive assessment of personality traits. The correct identification of personality disorders and their subtypes is critical for planning the therapeutic approach, including pharmacotherapy and psychological management.

  10. Marcha em pontas idiopática em idade pediátrica

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    Sara Domingues

    2016-03-01

    Full Text Available A marcha em pontas tem uma incidência de 7-24% na população pediátrica em geral e é uma causa relativamente frequente de referenciação à consulta de neurologia pediátrica. A marcha em pontas idiopática ocorre em crianças saudáveis, sem espasticidade e com reflexos osteotendinosos normais; é evidente desde o início da marcha autónoma, sempre bilateral e não progressiva. A sua etiologia é desconhecida, pelo que se trata de um diagnóstico de exclusão. Assim, na avaliação destas crianças é essencial estar alerta para sinais sensoriais ou motores, pois este padrão de marcha pode ser o primeiro sinal de patologia tal como paralisia cerebral, distrofia muscular congénita ou perturbação do espectro do autismo. As opções terapêuticas passam por tratamentos conservadores, como fisioterapia, utilização de calçado formativo, talas ou ortóteses, ou tratamentos mais invasivos, como uso de gessos seriados, aplicação de toxina botulínica ou cirurgia. Neste artigo de atualização pretende-se: abordar alguns aspetos epidemiológicos e fisiopatológicos, rever a apresentação clinica e diagnósticos diferenciais e propor orientações para o seguimento e tratamento em idade pediátrica.

  11. Indicativo de transtorno do desenvolvimento da coordenação de escolares com idade entre 7 e 10 anos

    Directory of Open Access Journals (Sweden)

    Juliana da Silva

    2013-03-01

    Full Text Available O objetivo do presente estudo foi caracterizar os participantes, de ambos os sexos, com idade entre 7 e 10 anos, quanto à presença do indicativo de Transtorno do Desenvolvimento da Coordenação - TDC. Participaram do estudo 406 crianças de uma escola municipal de São José/SC, com idades entre 7 e 10 anos, sendo 231 meninas e 175 meninos. As avaliações motoras e o indicativo de TDC foram realizados tendo como referência o Movement Assessment Battery for Children - primeira edição (MABC-1; HENDERSON; SUGDEN, 1992. A prevalência do indicativo de TDC foi de 11,1%, valor este considerado elevado quando comparado aos divulgados em pesquisas internacionais, porém semelhante aos percentuais encontrados em estudos realizados no Brasil.

  12. Qualidade de pintos em função do microclima, tempo de espera e idade de matrizes

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    Juliano R. de Camargo

    2015-11-01

    Full Text Available RESUMOPropôs-se avaliar a influência das condições microclimáticas do tempo de espera na sala de pintos do incubatório sobre a qualidade final dos pintos de um dia, oriundos de matrizes de diferentes idades. Foi mensurada a massa de 1440 ovos férteis, divididos em três lotes de 480 ovos cada um referentes às idades de matrizes (46, 54 e 64 semanas. Após o nascimento os pintos foram selecionados, sexados e subdivididos nas três idades de matrizes e em três tempos de espera (0, 14 e 28 h. Também foram instalados dataloggers na sala de espera e nas caixas de pintos para o monitoramento da temperatura do ar, umidade relativa e entalpia específica. O delineamento experimental utilizado foi inteiramente casualizado em esquema fatorial 2 x 3 x 3 com 50 repetições. As variáveis respostas analisadas foram: massa corporal dos pintos, temperatura cloacal, temperatura superficial média e frequência respiratória. O tempo de espera e as condições microclimáticas da sala de pintos do incubatório influenciaram no conforto térmico dos pintos. O melhor tempo de espera dos pintos foi o de 0 h. O maior percentual de perda de massa dos pintos devido ao tempo de espera foi observado nos pintos oriundos de matrizes com 54 semanas de idade.

  13. Idade de ocorrência da menopausa natural em mulheres brasileiras: resultados de um inquérito populacional domiciliar

    Directory of Open Access Journals (Sweden)

    Adriana Orcesi Pedro

    Full Text Available Realizou-se um estudo descritivo e exploratório de corte transversal, de base populacional, com o objetivo de estudar a idade à menopausa e seus fatores associados e características sócio-culturais, demográficas e econômicas em mulheres climatéricas, residentes no Município de Campinas, Estado de São Paulo. Selecionaram-se, através de amostragem por conglomerados, 456 mulheres, na faixa etária de 45-60 anos de idade. Os dados foram coletados através de entrevistas domiciliares, com um questionário estruturado e pré-testado. O questionário foi o resultado da adaptação, feita pelos autores, de questionários fornecidos pela Fundação Internacional de Saúde/Sociedade Internacional de Menopausa e pela Sociedade Norte-Americana de Menopausa. Para análise dos dados, foi utilizada a curva de sobrevivência pelo método de Tabela de Vida para estimar a taxa acumulada de mulheres na menopausa natural, e para determinar os fatores associados à idade da menopausa foi utilizada a análise de regressão logística de Cox. A média etária da ocorrência da menopausa natural foi de 51,2 anos. Não houve associação entre os fatores estudados com a idade à menopausa natural.

  14. Idade de ocorrência da menopausa natural em mulheres brasileiras: resultados de um inquérito populacional domiciliar

    Directory of Open Access Journals (Sweden)

    Pedro Adriana Orcesi

    2003-01-01

    Full Text Available Realizou-se um estudo descritivo e exploratório de corte transversal, de base populacional, com o objetivo de estudar a idade à menopausa e seus fatores associados e características sócio-culturais, demográficas e econômicas em mulheres climatéricas, residentes no Município de Campinas, Estado de São Paulo. Selecionaram-se, através de amostragem por conglomerados, 456 mulheres, na faixa etária de 45-60 anos de idade. Os dados foram coletados através de entrevistas domiciliares, com um questionário estruturado e pré-testado. O questionário foi o resultado da adaptação, feita pelos autores, de questionários fornecidos pela Fundação Internacional de Saúde/Sociedade Internacional de Menopausa e pela Sociedade Norte-Americana de Menopausa. Para análise dos dados, foi utilizada a curva de sobrevivência pelo método de Tabela de Vida para estimar a taxa acumulada de mulheres na menopausa natural, e para determinar os fatores associados à idade da menopausa foi utilizada a análise de regressão logística de Cox. A média etária da ocorrência da menopausa natural foi de 51,2 anos. Não houve associação entre os fatores estudados com a idade à menopausa natural.

  15. 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

  16. Crianças de dois anos de idade como coconstrutoras de cultura

    Directory of Open Access Journals (Sweden)

    Niina Rutanen

    2009-09-01

    Full Text Available De que maneira a cultura é coconstruída no nível micro das interações diárias em uma creche? O que é a “cultura” que está sendo construída, quem são os construtores e como o fazem? Este artigo se baseia em um estudo de caso de interação de crianças de dois anos de idade. Para o estudo, gravações em vídeo foram feitas duas vezes por mês durante um período de sete meses em uma creche na Finlândia. Nas sessões de gravação, as crianças recebiam alguns objetos para brincar. Quatro sessões foram selecionadas para a análise qualitativa. Durante a primeira sessão, as crianças produziram uma contracultura às tentativas da professora de estruturar a situação. Gestos, posturas e verbalizações entre as crianças surgiram de movimentos inicialmente aleatórios. O significado e as funções dessas posturas, movimentos e sons mudaram durante o andamento das ações. Alguns dos movimentos e verbalizações foram restabelecidos e mais elaborados nas sessões de gravação seguintes. As circunscrições para as ações foram constantemente negociadas verbalmente e não verbalmente entre as crianças e os adultos. A cultura institucional mais ampla da educação infantil não constituía uma estrutura passiva externa ao andamento das ações, mas ganhava concretude nas situações do aqui-e-agora. As expectativas e intenções dos adultos materializavam-se nas iniciações e nos ajustes do ambiente e canalizavam as possibilidades de ação das crianças. Baseando-se nisso, as crianças coconstruíam movimentos e significados novos fora da esfera de expectativa dos adultos.

  17. Desenvolvimento da camomila, rendimento e qualidade do óleo essencial em diferentes idades de colheita

    Directory of Open Access Journals (Sweden)

    W. Amaral

    2014-06-01

    Full Text Available A camomila é uma planta herbácea, anual e aromática com várias propriedades medicinais. No Brasil, vem sendo cultivada em área representativa na região Sul devido, principalmente, às exigências climáticas da espécie, e por ter sido introduzida por imigrantes europeus nesta região. A colheita da camomila é realizada em várias colheitas, contudo, a idade adequada da planta para o início desta atividade, objetivado a maior produção de capítulos florais, bem como o rendimento e qualidade de óleos essenciais, ainda não foi determinada para a espécie. Neste trabalho, investigou-se o efeito de diferentes épocas de colheita no desenvolvimento de capítulos florais e no acúmulo e qualidade do óleo essencial da camomila. O experimento foi conduzido no município de Piraquara (PR. O delineamento experimental foi inteiramente casualizado, com cinco tratamentos (85, 92, 99, 106 e 113 dias após a emergência das plântulas e cinco repetições. Após cada colheita, avaliou-se o acúmulo de massa seca de capítulos, rendimento, produção e composição do óleo essencial. A extração de óleo foi realizada por hidrodestilação e as amostras analisadas por cromatografia gasosa. Concluiu-se que aos 85 dias após a emergência (DAE os capítulos apresentaram maior rendimento de óleo. Porém, após três semanas ocorreu a maior produção de massa de capítulos, resultando em maiores médias de produtividade de óleo essencial. A partir de 113 DAE houve redução do rendimento de óleo essencial e no teor de alguns constituintes.

  18. Fatores associados à dislipidemia em crianças de 4 a 7 anos de idade

    Directory of Open Access Journals (Sweden)

    Taís Cristina Araújo Magalhães

    2015-02-01

    Full Text Available Objetivo: Avaliar o perfil lipídico e fatores associados à dislipidemia em crianças. Métodos: Estudo transversal que avaliou crianças de 4 a 7 anos acompanhadas nos primeiros meses de vida por um Programa de Extensão da Universidade Federal de Viçosa, Minas Gerais. Foram consideradas as dosagens de colesterol total, lipoproteína de alta densidade, lipoproteína de baixa densidade e triglicerídeos. Foram estudadas variáveis possivelmente associadas ao perfil lipídico, sendo elas variáveis maternas, sociodemográficas e aquelas associadas à criança. Foram realizadas análises bivariada e multivariadas, sendo as últimas por meio de regressão logística múltipla. Resultados: A amostra foi constituída por 185 crianças, de ambos os sexos. Observou-se que 46,5% (n=86 apresentaram valores aumentados de colesterol total, 9,2% (n=17 de lipoproteína de baixa densidade e 4,9% (n=9 de triglicerídeos. Com relação à lipoproteína de alta densidade, 35,1% (n=65 apresentaram valores abaixo do desejável. Demonstrou associação independente com o perfil lipídico das crianças a renda per capita, escolaridade materna e idade materna (associando-se à lipoproteína de baixa densidade e o excesso de peso, que se associou a maiores prevalências de alterações em triglicerídeos. Conclusão: Foram observadas altas prevalências de dislipidemias. Condições sociodemográficas e estado nutricional demonstraram influenciar, também em crianças, a ocorrência de dislipidemias, as quais são citadas como fatores de risco para as doenças cardiovasculares. Revela-se a importância de se estudar esses fatores desde a infância, realizando-se estudos com outras faixas etárias que verifiquem a prevalência e fatores associados, de forma a promover o cuidado com a saúde desse grupo populacional.

  19. Enxertia de fruteira-pão em função da idade do porta-enxerto

    Directory of Open Access Journals (Sweden)

    Alberico Raimundo da Silva Santana

    2014-12-01

    Full Text Available A fruteira-pão (Artocarpus altilis var. apyrena é uma Moraceae de alto valor nutritivo, com ampla distribuição no Brasil. O tipo sem sementes é comumente propagado por estaca de raiz, processo geralmente lento. O trabalho objetivou avaliar o método da enxertia para propagação de fruteira-pão em função da idade do porta-enxerto. Os porta-enxertos foram obtidos de fruteira-pão A. altilis com sementes, e o método de enxertia empregado foi o de garfagem de topo em fenda cheia. O delineamento experimental foi o inteiramente casualizado, com quatro tratamentos (constituídos por porta-enxertos de dois, quatro, seis e oito meses de idade, cinco repetições e 10 plantas por parcela. Foram avaliados o crescimento dos porta-enxertos, a partir do diâmetro do caule, e a altura da planta, e, após a enxertia, as porcentagens de pegamento aos 30 dias e de sobrevivência dos enxertos, número de brotos e de folhas do enxerto e o comprimento do maior broto, aos 90 dias após a enxertia. A enxertia por garfagem no topo em fenda cheia é viável para produção de mudas de fruteira-pão, proporcionando porcentagem de pegamento entre 76% e 92%, independentemente da idade do porta-enxerto. No entanto, verificou-se que o percentual de sobrevivência do enxerto (72% com os porta-enxertos com quatro meses e o diâmetro médio do caule de 10,52 mm foram superiores aos das demais idades. Houve pouca influência da idade do porta-enxerto para o número de brotos e de folhas, porém porta-enxertos com oito meses proporcionaram maior comprimento de broto.

  20. 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.

  1. 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...

  2. 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...

  3. 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.

  4. 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.

  5. 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.

  6. 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...

  7. 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.

  8. 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.

  9. 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.

  10. 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.

  11. 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.

  12. 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.

  13. 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®

  14. 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.

  15. 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.

  16. 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.

  17. 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.

  18. 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.

  19. 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 ...

  20. Relato de uma experiência de ensino de língua italiana para a terceira idade: desconstruindo concepções e arquitetando uma nova visão de mundo

    National Research Council Canada - National Science Library

    Sabrina de CAssia Martins

    2017-01-01

    ... results from the experience of teaching Italian to older students, and it aims to spotlight the motivating factors that brought these learners to foreign language lessons, and also their beliefs...

  1. 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)

  2. Pré-vestibulares alternativos: da igualdade à eqüidade Alternative courses for college entrance examination and higher education access: from equality to equity

    Directory of Open Access Journals (Sweden)

    Eleny Mitrulis

    2006-08-01

    Full Text Available Este artigo examina as crescentes demandas por acesso ao ensino superior em período em que se assiste a um deslizamento do debate sobre igualdade de oportunidades do plano da educação obrigatória para o terreno da educação superior. Representando os interesses dos novos grupos de concluintes de educação básica, proliferaram, a partir do final dos anos 90, dentro de movimentos sociais voltados para segmentos desassistidos da população, cursos preparatórios ao ensino superior, gratuitos e sem fins lucrativos. No âmbito das universidades públicas do Estado de São Paulo, igualmente sensíveis às urgências sociais da inclusão, registram-se também ações favoráveis ao acesso e à permanência desses segmentos sociais nos cursos oferecidos. O artigo analisa as ambigüidades e as aberturas presentes em programas preparatórios ao ensino superior, tomando como referência o Programa Pró-Universitário, voltados aos alunos da série terminal da educação básica, pertencentes à rede estadual de ensino, desenvolvido pela Universidade de São Paulo em parceria com a Secretaria de Estado da Educação. Traz uma análise do perfil dos alunos participantes e uma reflexão sobre os efeitos desse tipo de iniciativa sobre a relação dos jovens com o saber e sobre a construção de suas identidades. Sugere que a ação afirmativa para a inclusão de jovens dos segmentos populares em instituições públicas de ensino superior requer uma proposta educativa na qual a socialização e a aprendizagem estejam intimamente ligadas. O domínio dos saberes preparatórios aos exames de acesso deixa de ser considerado apenas pelo valor instrumental e adquire outros significados como uma nova maneira de ver o mundo, relacionar-se consigo mesmo e com o outro.This work explores the growing demands for increasing access to higher education at a time when discussions on equality of opportunities at the level of compulsory education are shifting to higher

  3. Trabalho feminino e saúde na terceira idade Women's work and health among Brazilian elderly

    Directory of Open Access Journals (Sweden)

    Luana Giatti

    2002-01-01

    Full Text Available O objetivo deste estudo é estimar e caracterizar a participação de idosas no mercado de trabalho e investigar diferenciais de saúde, segundo sua inserção nesse mercado, após considerar a influência de fatores sociodemográficos. O estudo incluiu 4.607 com 65 anos e mais, residentes em dez regiões metropolitanas brasileiras e participantes da PNAD/98. Foram definidas as categorias: trabalhando, aposentada e outra. A análise incluiu o qui-quadrado e o odds ratio estimado através de regressão logística multinomial. Quase 10% das mulheres trabalhavam, 42% eram aposentadas e 48% não trabalhavam nem eram aposentadas. As idosas ocupadas eram mais jovens, tinham maior renda, e de 4 a 7 anos de escolaridade. O fato de estar trabalhando esteve associado à melhor percepção da própria saúde, menor relato de doenças crônicas, plano privado de saúde, menor relato de consulta e internação hospitalar, melhores indicadores de autonomia e mobilidade física e maior freqüência de consulta odontológica. A permanência das idosas na vida ativa é inferior à dos homens brasileiros no mesmo período. Os diferenciais de saúde relacionados ao trabalho são mais acentuados entre as mulheres. É fundamental determinar se os diferenciais de saúde observados entre idosas, também são encontrados nas mulheres em idade ativa.The objective of this study is to estimate and describe the participation of aged women in the labour market, and to investigate health differentials according to their working position, after considering the influence of social and demographic factors. This study comprises 4.607 females aged 65 or more, residents in 10 Brazilian metropolitan regions and participants of PNAD conducted in 1998. The following working categories have been defined: working, retired and other. The analysis was based on qui-square tests and odds ratios were obtained by multinomial logistic regression. Almost 10% of the aged women worked, 42% were

  4. Produção do Superprecoce a Partir de Bezerros Desmamados aos 72 ou 210 Dias de Idade

    Directory of Open Access Journals (Sweden)

    Restle João

    2002-01-01

    Full Text Available O experimento foi conduzido com o objetivo de avaliar o desempenho em confinamento, dos 210 aos 408 dias de idade, de bezerros previamente desmamados aos 72 (T72 ou 210 (T210 dias. Foram utilizados 36 machos não castrados da raça Braford (5/8 Hereford 3/8 Nelore. O peso médio no início do experimento foi de 209 kg (T72 e 192 kg (T210. O confinamento compreendeu 30 dias de adaptação dos animais e 168 dias de avaliação, sendo dividido em quatro períodos de 42 dias. A relação volumoso:concentrado foi de 60:40 para o 1º e 2º períodos, 50:50 para o 3º período e 45:55 para o 4º período. Não houve interação entre idade de desmame e período de avaliação em confinamento para os parâmetros relativos aos consumos médios por animal de matéria seca (CMS e de energia digestível (CED, expressos em kg/dia e Mcal/dia (CMSD e CEDD, por 100 kg de peso vivo (CMSP e CEDP e por unidade de tamanho metabólico (CMSM e CEDM, ao ganho de peso médio diário (GMD, à conversão alimentar (CA e eficiência energética (EE. Animais desmamados aos 210 dias apresentaram maiores CMSP (2,25 contra 2,07% PV e CEDP (7,05 contra 6,48% PV em relação aos animais desmamados ao 72 dias de idade. Não houve diferença no CMSD (6,75 contra 6,98 kg/dia, no GMD (1,066 contra 1,074 kg/dia, na eficiência de conversão da matéria seca (6,42 contra 6,72 kg de MS/kg ganho de PV e da energia digestível consumida (20,18 contra 21,13 Mcal/kg ganho de PV em ganho de peso vivo para os animais desmamados aos 72 ou 210 dias de idade, respectivamente. Os pesos de abate e de carcaça quente foram similares entre as duas idades, sendo, respectivamente, de 424 e 232 kg para os animais do T72 e de 406 e 221 kg para dos T210. Os resultados mostram que animais desmamados aos 72 dias de idade apresentaram desempenho durante a terminação, pesos de abate e de carcaça similares aos desmamados aos 210 dias.

  5. 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.

  6. 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.

  7. 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.

  8. 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...

  9. 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.

  10. 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.

  11. Microclima, idade das matrizes e tempo de estocagem influenciando nas respostas produtivas de ovos férteis

    Directory of Open Access Journals (Sweden)

    Aérica C. Nazareno

    2014-11-01

    Full Text Available Objetivou-se, com esta pesquisa, avaliar as condições microclimáticas da sala de ovos e sua influência na perda de água dos ovos férteis em função das diferentes idades de matrizes e tempos de estocagem. A sala de ovos apresentava as seguintes dimensões: 15 x 9,90 x 2,8 m, climatizada por quatro aparelhos de ar condicionados. Foram selecionadas três diferentes idades de matrizes e três intervalos de tempo de estocagem. Quando as aves atingiam as três idades eram coletados 1440 ovos, foram coletados a massa (kg de 140 ovos individualizados de cada tratamento, durante sua entrada e saída da sala utilizando-se uma balança semianalítica para avaliação da perda de água dos ovos. A avaliação microclimática da sala foi realizada em intervalos de 10 min. por meio do registro de temperatura (°C, umidade relativa (% e entalpia específica (kJ kg-1 de ar seco utilizando-se 19 dataloggers. O delineamento experimental utilizado foi inteiramente aleatorizado com esquema fatorial 3 x 3. As condições microclimáticas da sala se mantiveram acima da faixa ideal e o verão foi o período mais quente. Os ovos oriundos de matrizes velhas e intermediárias com o tempo de estocagem de 50-52 h apresentaram as maiores perdas de água.

  12. Relação entre idade e variação da flexibilidade de bailarinas

    Directory of Open Access Journals (Sweden)

    Aline Huber da Silva

    2008-10-01

    Full Text Available O objetivo deste estudo foi verificar se o comportamento da flexibilidade, após 8 semanas de aplicação da técnica de alongamento por Facilitação Neuromuscular Proprioceptiva em bailarinas, tem relação com suas idades. A amostra foi obtida de forma intencional, composta por 11 bailarinas na faixa etária de 13 a 16 anos. Realizou-se avaliação da flexibilidade angular dos movimentos de flexão (com o joelho estendido, abdução e rotação externa do quadril através da goniometria e da flexibilidade linear com a Caixa de Sentar e Alcançar de Wells, antes e após o período experimental de oito semanas, com duas intervenções semanais, utilizando a técnica de FNP. Para análise, usou-se estatística descritiva, teste t e correlação linear de Pearson. Adotou-se significância de 5%. Somente a variação da rotação externa e da Caixa de Sentar e Alcançar, durante o período experimental, apresentaram correlação estatisticamente significativa com a idade das bailarinas, porém, essa correlação ainda assim foi bastante fraca. Pode-se perceber que praticamente não houve relação entre a variação da flexibilidade com a idade da amostra.

  13. A Idade e Natureza da Fonte do Granito do Moinho, Faixa Ribeira, Sudeste do Estado de São Paulo

    Directory of Open Access Journals (Sweden)

    Colombo Celso Gaeta Tassinari

    2004-04-01

    Full Text Available Este trabalho apresenta novos dados geocronológicos U-Pb SHRIMP em zircões e Sm-Nd em rocha total do Granito doMoinho, que ocorre nas imediações da cidade de Nazaré Paulista, Estado de São Paulo. Este granito apresenta característicasin- a tardi-tectônica em relação à Orogenia Brasiliana e é intrusivo nas seqüências mesoproterozóicas do Grupo Serra doItaberaba, no segmento central da Faixa de Dobramentos Ribeira. Adicionalmente, foram reavaliados dados isotópicos de Pbobtidos em amostras de rocha total e feldspatos potássicos disponíveis na literatura. A idade U-Pb SHRIMP obtida emmonocristais de zircões ígneos do granito foi de 620 ± 11 Ma, sendo interpretada como a época de cristalização desta rocha.As idades modelo Sm-Nd obtidas situaram-se entre 2,0 e 1,9 Ga, mostrando que o magma foi produzido por fusão parcial derochas pré-existentes, derivadas do manto superior no Paleoproterozóico. As composições isotópicas de Pb das amostras doGranito do Moinho indicam, a exemplo dos isótopos de Nd, uma fonte também crustal e com participação de rochas doGrupo Serra do Itaberaba, de idade mesoproterozóica.

  14. 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.

  15. 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.

  16. 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.)

  17. 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.

  18. 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.

  19. A influência da idade e da escolaridade sobre a experiência empática de adultos

    OpenAIRE

    Vanessa Dordron de Pinho; Conceição Santos Fernandes; Eliane Mary de Oliveira Falcone

    2011-01-01

    Atualmente, os teóricos começam a compartilhar uma visão da experiência empática humana como um fenômeno multidimensional influenciado por diversos aspectos, dentre eles, a idade e a escolaridade. No presente estudo, investigou-se as relações entre a habilidade social empática e essas duas variáveis sociodemográficas, em 537 participantes adultos. A habilidade empática foi estudada em quatro dimensões, que correspondem aos quatro fatores que compõem o instrumento utilizado, o Inventário de Em...

  20. Infecção Urinária em Idade Pediátrica - Estudo Retrospectivo

    OpenAIRE

    Sarmento, Alzira; Garrido,Cristina; Maia, Iris; Maciel, Idalina

    2014-01-01

    A inespecificidade de sintomas e o maior risco de cicatriz renal fazem com que as Infecções do Tracto Urinário (ITU) assumam especial importância na idade pediátrica.Procedeu-se à análise retrospectiva dos processos clínicos das crianças internadas por ITU, no Serviço de Pediatria do Hospital Santa Luzia, no período de Janeiro de 1999 a Junho de 2001.Os objectivos traçados foram: caracterizar a população em causa, avaliar as sensibilidades dos agentes causais aos antibióticos testados, avalia...

  1. Bruxismo noturno em crianças de 8 a 10 anos de idade: fatores psciológicos associados

    OpenAIRE

    Drumond,Clarissa Lopes

    2014-01-01

    Justificativa: considerando-se que a etiologia do bruxismo noturno ainda não foi completamente esclarecida, torna-se necessário o desenvolvimento de estudos de base populacional que permitam a identificação dos fatores associados a esta desordem. Objetivo: verificar a prevalência e os fatores associados ao bruxismo noturno em escolares brasileiros de 8 a 10 anos de idade. Métodos: realizou-se um estudo transversal com uma amostra representativa de 473 escolares, matriculados em escolas públic...

  2. Familia e deficiencia : o significado de conviver e crescer junto a uma pessoa portadora de deficiencia mental na idade adulta

    OpenAIRE

    Marta Fuentes Rojas

    2001-01-01

    Resumo: Esta pesquisa levanta alguns elementos que permitem criar subsídios para auxiliar o profissional que trabalha com a deficiência mental e para melhorar o atendimento a estas famílias. Os elementos foram identificados das experiências cotidianas de seis famílias, cadauma com um membroportador de deficiência mental na idade adulta, levantando dados sobre: a construção do conceito de deficiência mental; as formas de agir e de reagir do portador de deficiência e dos demais membros do grupo...

  3. Padrões motores de escolares de oito a nove anos de idade da cidade de Santa Rosa, RS

    OpenAIRE

    Loi, Luiz Serafim de Mello

    1999-01-01

    Dissertação (mestrado) - Universidade Federal de Santa Catarina, Centro de Desportos. O desenvolvimento motor é um assunto que necessita maiores estudos, haja vista a importância cada vez maior do desenvolvimento pleno da criança, desde os primeiros anos de vida. Este estudo utilizando como Marco Referencial Teórico (MRT) o modelo de desenvolvimento motor de Gallahue & Ozmun (1998) teve por objetivo verificar o perfil motor de escolares de oito e nove anos de idade, da cidade de Santa Rosa...

  4. GESTÃO DE PROGRAMAS INTERDISCIPLINARES PARA A TERCEIRA IDADE EM UNIVERSIDADES PÚBLICAS DE FLORIANÓPOLIS

    OpenAIRE

    Silva, Flora Moritz Da; Silva, André Tiago Dias da; Costa, Alexandre Marino; Rocha, Rudimar Antunes da

    2014-01-01

    O objetivo deste artigo é descrever os processos de gestão de Programas Interdisciplinares para a Terceira Idade das universidades públicas de Florianópolis, “Universidades da Terceira Idade”, movimento que desde a década de 70 vem crescendo no mundo. Apesar de o Brasil contar com mais de 200 projetos deste tipo e uma crescente população idosa, há poucos recursos destinados a tais programas, bem como pouca pesquisa sobre a gestão dos mesmos. Para tanto, realizou-se um levantamento bibliográfi...

  5. Perfil motor de escolares de 7 a 10 anos de idade com indicativo de Desordem Coordenativa Desenvolvimental (DCD)

    OpenAIRE

    2010-01-01

    Este estudo teve como objetivo analisar o perfil motor de escolares de 7 a 10 anos de idade com indicativo de Desordem Coordenativa Desenvolvimental. Participaram do estudo 380 crianças provindas de escolas da rede pública de ensino da parte continental da cidade de Florianópolis –SC –Brasil. Esta pesquisa foi aprovada pelo Comitê de Ética em Pesquisa em Seres Humanos da UDESC. Para a identificação de dificuldades motoras foi utilizado o Movement Assessment Battery for Children (MABC-2) e par...

  6. Polifarmácia em Idosos do Programa Universidade Aberta à Terceira Idade da Universidade Federal de Pernambuco

    OpenAIRE

    Alves, Niedja Maria Coelho

    2014-01-01

    Polifarmácia é o uso de dois ou mais medicamentos para o mesmo ou vários problemas de saúde. Sua prática é considerada um tipo de uso irracional de medicamentos, podendo acarretar reações adversas e interações medicamentosas, principalmente em idosos, os mais vulneráveis a estes problemas. Descrever a polifarmácia em idosos inscritos no Programa Universidade Aberta à Terceira Idade (UnATI) da Universidade Federal de Pernambuco (UFPE). Estudo do tipo transversal descritivo, realizado com 159 a...

  7. 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 ...

  8. 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...

  9. 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.

  10. 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 ...

  11. 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.

  12. 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

  13. Diagnóstico de saúde das mulheres em idade fértil de Sergipe

    Directory of Open Access Journals (Sweden)

    Alzira Maria D'avila Nery Guimarães

    1996-03-01

    Full Text Available Relato parcial de uma pesquisa realizada pela Secretária de Estado da Saúde em parceria com o UNICEF, intitulado de Diagnóstico Matemo-lnfantil cio Estado de Sergipe. Nesta pesquisa as autoras realizam uma abordagem parcial sobre a saúde das mulheres em idade fértil. Objetivo: Medir por amostragem a nível estadual os indicadores: estado civil, idade da menarca, início da vida sexual, gravidez, abortos, prevenção do câncer cérvico-uterino e mama, anticoncepção e utilização dos serviços de saúde. Os resultados foram coletados através da aplicação de um formulário estruturado, abrangendo variáveis préconcepcionais, biológicas e sociais. Os dados obtidos fornecem subsídios para ampla discussão sobre a saúde das mulheres em Sergipe.

  14. Transporte de ovos férteis: Influência das idades das matrizes, tempos de estocagem e das estradas

    Directory of Open Access Journals (Sweden)

    Aérica C. Nazareno

    2014-03-01

    Full Text Available Propôs-se, com esta pesquisa, avaliar a influência de diferentes idades das matrizes e tempos de estocagem no número de ovos trincados durante a operação de transporte em diferentes estradas. A pesquisa foi conduzida na empresa integradora avícola em Mogi-Mirim - SP, por meio do acompanhamento de três carregamentos em diferentes estações do ano (primavera, verão e outono. Foi utilizado um caminhão climatizado do tipo baú com capacidade para 592 caixas de ovos. Foram registrados, por meio de quatro acelerômetros, os níveis de vibração (m s-2 e choques em percursos realizados nas estradas de terra e asfalto. O número de ovos trincados foi obtido por meio da contabilização de 18 caixas de ovos transportadas que apresentavam três idades de matrizes e três tempos de estocagem, pelo método visual. Foi utilizado o delineamento experimental inteiramente aleatorizado com esquema fatorial 3 x 3. Conclui-se que as matrizes velhas e intermediárias apresentaram o maior número de ovos trincados; os maiores níveis de vibração e choques da carga ocorreram no sentido horizontal enquanto a estrada de asfalto ofereceu as piores condições para o transporte de ovos.

  15. A influência da idade e da escolaridade sobre a experiência empática de adultos

    Directory of Open Access Journals (Sweden)

    Vanessa Dordron de Pinho

    2011-08-01

    Full Text Available Atualmente, os teóricos começam a compartilhar uma visão da experiência empática humana como um fenômeno multidimensional influenciado por diversos aspectos, dentre eles, a idade e a escolaridade. No presente estudo, investigou-se as relações entre a habilidade social empática e essas duas variáveis sociodemográficas, em 537 participantes adultos. A habilidade empática foi estudada em quatro dimensões, que correspondem aos quatro fatores que compõem o instrumento utilizado, o Inventário de Empatia (IE: Tomada de Perspectiva (TP, Flexibilidade Interpessoal (FI, Altruísmo (Al e Sensibilidade Afetiva (SA. Os resultados indicaram correlações significativas do ponto de vista estatístico entre idade e dois aspectos da empatia: altruísmo e sensibilidade afetiva. Os grupos de escolaridade se diferenciaram quanto à flexibilidade interpessoal e ao altruísmo. Através deste artigo é possível hipotetizar que as variáveis estudadas estão relacionadas à empatia, corroborando estudos anteriores que apontam como variáveis cognitivas caminham juntas com o desenvolvimento e podem ser afetadas pelo aprimoramento educacional.

  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. Ocorrência de enteroparasitas na população geronte de Nova Olinda do Norte Amazonas, Brasil Occurrence of enteroparasites in the elderly population of Nova Olinda do Norte, Amazonas, Brazil

    Directory of Open Access Journals (Sweden)

    Ana Felisa Hurtado-Guerrero

    2005-12-01

    Full Text Available Foi realizado um estudo para avaliar a prevalência de enteroparasitas em um grupo de idosos ribeirinhos, moradores do Município de Nova Olinda do Norte, Estado do Amazonas Brasil, no período de abril e agosto de 1999. Por meio de um estudo de corte transversal foram analisados 81 exames, através do método de Sedimentação Espontânea (Método de Hoffman et al., 1934. Foi constatada positividade em 72,8% dos idosos, predominando o monoparasitismo (43,2%. Os helmintos foram os mais freqüentes (70,4%, destacando-se: Ascaris lumbricoides (35,2%, Trichuris trichiura (16,0%, Ancylostoma duodenale (9,0% e Strongyloides stercoralis (9,0%. Dentre os protozoários (29,5%, a ocorrência de Entamoeba coli foi de 18,2%, Giárdia lamblia de 7,0% e Entamoeba histolytica 4,5%. Não houve associação estatisticamente significativa entre sexo e grau de parasitismo e entre faixas etárias e condição parasitária. Estes resultados evidenciam um quadro de alta prevalência de parasitas intestinais nesta população e discordam dos reportados por outros pesquisadores quando afirmam que a intensidade da infestação por parasitas diminui na idade avançada. Os achados anteriores exigem das autoridades governamentais medidas de controle e educação para melhorar a qualidade de vida desses idosos, considerando a grave repercussão que esses parasitas tem no estado nutricional dos gerontes de baixa renda.A study was carried out to determine the prevalence of enteroparasites attacking elderly people living in a riverside city of the Municipal district of Nova Olinda do Norte, Amazonas State Brazil. In this cross sectional study were examined the faecal material from 81 elderly people using the method of spontaneous sedimentation (Hoffman et al., 1934. It was found a positiveness in 72,8% of the elderly people examined, predominating the mono parasitism (43,2%. The helminths were more frequents (70,3%: Ascaris lumbricoides (35,2%, Trichuris trichiura (16

  12. 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

  13. Symphysis-fundal height curve in the diagnosis of fetal growth deviations Curva de altura uterina por edad de gestación y diagnóstico de desvíos del crecimiento fetal Curva de altura uterina por idade gestacional e diagnóstico de desvios do crescimento fetal

    Directory of Open Access Journals (Sweden)

    Djacyr Magna Cabral Freire

    2010-12-01

    ência brasileira por idade gestacional. Uma subamostra de 122 casos com pesos neonatais obtidos até sete dias depois da estimativa do peso fetal, a classificação da altura uterina foi comparada com a curva de Lubchenco como padrão-ouro. A sensibilidade, a especificidade e os valores preditivos positivo e negativo foram calculados. Para comparar o desempenho da sensibilidade entre ambas as curvas de altura uterina, utilizou-se o teste χ2 de McNemar. RESULTADOS: A sensibilidade da nova curva para a detecção de fetos pequenos para a idade gestacional foi de 51,6%, enquanto a da curva do padrão-ouro foi significativamente menor (12,5%. Na subamostra que teve o peso neonatal como padrão-ouro, a sensibilidade da nova curva de referência foi de 85,7%, enquanto a do Ministério da Saúde exibiu 42,9% de sensibilidade para a detecção de fetos pequenos para a idade gestacional. CONCLUSÕES: A capacidade diagnóstica da nova curva de referência para detectar fetos pequenos para a idade gestacional foi significativamente melhor do que a da curva recomendada pelo Ministério da Saúde.

  14. Idade de desmame e suplementação no desenvolvimento e em características de carcaças de novilhos de corte

    Directory of Open Access Journals (Sweden)

    Almeida Luciane Salgueiro Pio de

    2003-01-01

    Full Text Available O experimento foi conduzido na Estação Experimental da Universidade Federal do Rio Grande do Sul, município de Eldorado do Sul, Brasil, a fim de avaliar o desempenho de 40 bezerros filhos de vacas cruzas Bos indicus x Bos taurus até os dois anos de idade, desmamados precocemente (DP, com média de idade de 91 dias e mínimo de 70 kg de peso vivo, ou desmamados à idade convencional (DC, média de 170 dias de idade e peso médio de 131,2 kg, suplementados (Su ou não (NSu com ração energético-protéica com 14% de proteína bruta e 75% de nutrientes digestíveis totais, durante 91 dias no primeiro inverno. O delineamento experimental utilizado foi o delineamento completamente casualizado. Os novilhos do DP foram mais leves até um ano de idade (DP=208,7 kg x DC=233,5 kg. Aos 18-20 meses de idade, os novilhos não eram mais estatisticamente diferentes em seus pesos vivos (DP=279,9 kg x DC=292,5 kg. Ao abate, os pesos vivos médios foram de 432,3 kg (DC e 414,0 kg (DP, não diferindo também no rendimento, acabamento, conformação e classificação das carcaças. O desmame precoce não impediu o desenvolvimento e o abate dos novilhos aos dois anos de idade. A suplementação no primeiro inverno não alterou o desempenho dos novilhos ao abate.

  15. 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.

  16. The rms-flux relation in accreting white dwarfs: another nova-like variable and the first dwarf nova

    CERN Document Server

    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.

  17. Perimetria computadorizada em pacientes de mais de 70 anos de idade Computerized perimetry in over 70-year-old patients

    Directory of Open Access Journals (Sweden)

    Maria Helena Mandello Carvalhaes

    2000-08-01

    Full Text Available Objetivo: Comparar os índices globais e o tempo do exame de campo visual computadorizado entre pacientes de mais de 70 anos e abaixo de 60 anos de idade. Método: Foram realizados exames de campo visual (Humphrey 24-2 em 56 pacientes com mais de 70 anos (88 olhos e em 23 pacientes com idade inferior a 60 anos (46 olhos. Comparou-se entre os grupos os índices globais, tempo de exame e confiabilidade, para o olho direito e esquerdo. Entre os pacientes com mais de 70 anos comparou-se exames confiáveis e não-confiáveis. Dos pacientes com exame confiável bilateral foi realizada comparação entre os índices globais e tempo de exame entre olho direito e esquerdo. Resultados: A média de idade dos pacientes de mais de 70 anos foi 77,7 ± 5 anos e dos abaixo de 60 anos de 50,0 ± 5 anos. Houve diferença estatística do "Pattern Standard Deviation" (OD p = 0,02 e OE p = 0,03, "Corrected Pattern Standard Deviation" (OD p = 0,02 e OE p = 0,44. Os pacientes de mais de 70 anos de idade necessitaram de um maior tempo para realização do exame (t acima de 70 anos OD= 11,8 ± 1,8min - t abaixo 60=11,1 ± 1,9min p = 0,04; t acima de 70 anos OE=11,4 ± 1,4 min - t abaixo 60 OE = 10,8 ± 1,8 min p = 0,009. Nos pacientes de mais de 70 anos de idade, os campos não-confiáveis apresentaram maiores valores de PSD e CPSD de forma estatisticamente significante. A comparação em casos dos pacientes com mais de 70 anos de idade com exames bilaterais não evidenciaram diferenças estatísticas para os todos índices globais e para o tempo de exame (pMD = 0,4; pPSD = 0,9; pSF = 0,68; pCPSD = 0,92; p tempo = 0,11. Conclusão: Observou-se um maior tempo de exame entre os pacientes com mais de 70 anos de idade e valores de PSD e CPSD estatisticamente mais elevados sugerindo uma maior variação da sensibilidade no campo visual destes pacientes.Purpose: To compare global indices and duration of automated visual field tests in geriatric patients and in patients below

  18. Comparação entre as curvas de crescimento do Centers for Disease Control and Prevention e da Organização Mundial da Saúde para lactentes com idade de seis a 12 meses Comparison between the Centers for Disease Control and Prevention and the World Health Organization growth curves for six to 12 months old infants

    Directory of Open Access Journals (Sweden)

    Bianca Sant'Anna Pires

    2010-12-01

    Full Text Available OBJETIVO: Comparar o estado nutricional de lactentes de ambos os sexos de acordo com a curva proposta pelo Centers for Disease Control and Prevention (CDC-2000 e com a nova curva de crescimento proposta pela Organização Mundial da Saúde (OMS-2006. MÉTODOS: Estudo longitudinal no qual foram acompanhadas crianças de ambos os sexos, nascidas a termo, com idade entre seis meses e um ano, em aleitamento materno predominante ou exclusivo. Os dados foram coletados por um único pesquisador por meio de ficha de atendimento nutricional composta por dados demográficos, antropométricos e sobre a alimentação da criança. Foram realizados testes de Wilcoxon e Friedman para comparar cada medida das curvas e analisar a variância, respectivamente. RESULTADOS: Da amostra final de 55 crianças, 51% (n=28 eram do sexo masculino. Os percentuais de eutrofia dos índices de peso por idade e de estatura adequada para idade de ambos os sexos apresentaram-se acima de 80%. Não houve diferença significante na classificação do estado nutricional, segundo as curvas utilizadas. A porcentagem de concordância das duas curvas em relação ao peso e à estatura foi de 98,2 e 96,4%, respectivamente. CONCLUSÕES: As curvas de crescimento da OMS-2006 e do CDC-2000 foram similares para classificar o estado nutricional de lactentes entre 6-12 meses em aleitamento materno.OBJECTIVE: Compare the nutritional status of male and female infants classified according to the growth curve proposed by the Center for Disease Control and Prevention (CDC-2000 and the new growth curve proposed by the World Health Organization (WHO-2006. METHODS: This longitudinal study enrolled children of 6-12 months old of both genders. They were born at term and exclusively or predominantly breastfed. A single researcher collected demographic, anthropometric and nutritional data. The Wilcoxon test was used to compare curves and the Friedman test was used to analyze the variance. RESULTS: Among the

  19. Exigência de metionina + cistina para frangas de reposição na fase cria de sete a 12 semanas de idade

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    P. D'Agostini

    2012-12-01

    Full Text Available Determinou-se a exigência de metionina + cistina para frangas de sete a 12 semanas de idade e verificou-se seu efeito sobre a fase de postura. O experimento foi dividido em duas fases, de cria e de produção, esta de 22 a 33 semanas de idade. Na primeira fase, utilizaram-se 640 aves - 50% Lohmann LSL e 50% Lohmann Brown - com sete a 12 semanas de idade, distribuídas em delineamento inteiramente ao acaso, em esquema fatorial 5x2 (porcentagem de met+cis e linhagem, com quatro repetições e 16 aves por repetição. As porcentagens de met+cis total estudadas foram 0,471; 0,541; 0,611; 0,681 e 0,751%. Ao atingirem 22 semanas de idade, 240 aves foram utilizadas para verificar o efeito residual das dietas fornecidas na fase de cria. A dieta fornecida nesta fase foi igual para todas as aves. As exigências de metionina + cistina para aves de reposição, leves e semipesadas, no período de sete a 12 semanas de idade, foram de 0,710 % de met+cis total (0,639% de met+cis digestível e 0,706% de met+cis total (0,635% de met+cis digestível, respectivamente.

  20. Caracterização de sujeitos com lesão cerebral adquirida em idade produtiva

    Directory of Open Access Journals (Sweden)

    Aline Sarturi Ponte

    Full Text Available RESUMO Objetivo: analisar as condições sociodemográficas e de saúde (inclusive os agravos neurológicos de sujeitos com LEA em idade produtiva, bem como suas condições pregressas e atuais de trabalho. Métodos: estudo de natureza descritiva e de abordagem quantitativa. Os dados foram coletados entre junho e dezembro de 2014, por meio de uma entrevista semiestruturada. Resultados: participaram do estudo 48 sujeitos com Lesão Cerebral Adquirida; a incidência entre o sexo masculino (52,1% e feminino (47,9% foi equilibrada; a média de idade, no momento da lesão, foi de 48,7 anos; 64,5% eram casados; 62,5% possuíam Ensino Fundamental Incompleto; a ocupação anterior à lesão mais frequente foi a de doméstica (18,7%; 47,9% dos sujeitos foram aposentados após a lesão, 6,3% voltaram ao trabalho, e 93,7% gostariam de retornar. Quanto aos comprometimentos neurológicos, 41,1% foram acometidos por Acidente Vascular Cerebral Isquêmico (52,1% apresentaram afasia, e 52,2% tiveram hemiplegia direita. A condição de saúde física de 60,4% foi considerada moderada; 58,3% avaliaram sua saúde mental como ruim; 60,4% nunca fumaram; e 93,7% pararam de ingerir álcool após a lesão. Notou-se, ainda, que 62,5% dos sujeitos eram acompanhados somente por fisioterapeutas e que 54,2% usavam algum recurso assistivo. Ademais, as atividades de lazer de 58,4% dos sujeitos estavam prejudicadas. Conclusão: a média de idade dos sujeitos deste estudo é inferior a outros estudos nacionais; o nível de escolaridade é baixo; as ocupações anteriores à lesão eram de baixo rendimento financeiro; e o índice de aposentadoria após a lesão foi alto. As sequelas neurológicas impactam, assim, negativamente a vida/saúde dos sujeitos, condição agravada pelo fato de os recursos terapêuticos serem incompletos.

  1. Falhas dos componentes externos do implante coclear: influência da idade e do tempo de uso

    Directory of Open Access Journals (Sweden)

    Alessandra Martins Pereira

    2014-10-01

    Full Text Available OBJETIVO: identificar quais são as falhas técnicas mais frequentes dos componentes externos do implante coclear e verificar a influência da idade do usuário e o tempo de uso do dispositivo nestas falhas.MÉTODOS: estudo retrospectivo, por meio da análise de 128 prontuários da Associação dos Deficientes Auditivos, Pais, Amigos e Usuários de Implante Coclear, que apresentaram alguma queixa no funcionamento do componente externo, no período de junho a agosto de 2011. Para análise dos dados foi realizada a análise descritiva dos componentes que apresentaram falha técnica, bem como das variáveis estudadas. Posteriormente, foi aplicada a estatística inferencial por meio do teste Kruskal-Wallis para verificar a influência da idade do paciente e tempo de uso do implante coclear com a falha apresentada, com nível de significância p< 0,05.RESULTADOS: os componentes que apresentaram mais falhas foram: antena externa (29,7%, seguida do compartimento de bateria (23,4%, processador de fala (14,10%, microfone (10,90%, cabos de transmissão (9,40%, controlador (6,30%, baterias (5,50% e carregador de baterias (0,80%. Não foi verificada influência do tempo de uso do implante coclear e a idade cronológica do paciente em relação às falhas apresentadas no presente estudo.CONCLUSÃO: os achados obtidos a partir do presente estudo podem auxiliar os profissionais da área na orientação sobre a manutenção destes componentes, mas as tendências aqui apresentadas não podem ser generalizadas para todo território nacional, pois estas foram analisadas em um número limitado de casos.

  2. 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.

  3. 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.

  4. 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.

  5. 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

  6. 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.

  7. 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]..

  8. 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.

  9. 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...

  10. 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 ...

  11. 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...

  12. 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.

  13. 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 ...

  14. 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.

  15. 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...

  16. Associação entre idade ao início da atividade sexual e subseqüente infecção por papilomavírus humano: resultados de um programa de rastreamento brasileiro Association between age at first sexual intercourse and subsequent human papillomavirus infection: results of a Brazilian screening program

    Directory of Open Access Journals (Sweden)

    Cecília Maria Roteli-Martins

    2007-11-01

    Full Text Available OBJETIVO: descrever a idade de início da atividade sexual (sexarca e a sua associação com a idade das mulheres com a infecção por papilomavírus humano (HPV e com as alterações citológicas no exame de papanicolaou. MÉTODOS: mulheres da população geral foram recrutadas para participar de um estudo de rastreamento de câncer cervical e lesões pré-malignas. Após a aplicação de questionário comportamental, foram submetidas ao rastreamento com gia cervical e teste para DNA de HPV de alto risco, por meio de Captura Híbrida 2. Este projeto faz parte do Latin American Screening Study, que envolve mulheres do Brasil e da Argentina, e os dados aqui apresentados referem-se aos centros brasileiros nas cidades de Porto Alegre, São Paulo e Campinas. RESULTADOS: de 8.649 mulheres entrevistadas, 8.641 relataram atividade sexual prévia e foram incluídas na análise. A média de idade no momento da entrevista foi de 38,1±11,04 anos, com início da atividade sexual em média aos 18,5±4,0 anos. Identificamos que a idade do início da atividade sexual aumenta de acordo com o aumento da faixa etária no momento da entrevista, isto é, mulheres mais novas relataram sexarca mais precoce que mulheres mais velhas (p ou = ASC-US (6,7% do que mulheres com sexarca em idade maior que a média (4,3% - OR=1,6 (IC95%=1,3-2,0; pPURPOSE: to investigate women’s age at their first sexual intercourse and its correlation with their present age, human papillomavirus (HPV infection and cytological abnormalities at Pap smear. METHODS: women from the general population were invited to be screened for cervical cancer and pre-malignant lesions. After answering a behavior questionnaire, they were submitted to screening with cervical cytology and high-risk HPV testing with Hybrid Capture 2 (HC2. This report is part of the Latin American Screening (LAMS study, that comprises centers from Brazil and Argentina, and the data presented herein refer to the Brazilian women

  17. Arterite de Takayasu com estenose de artéria renal diagnosticada em paciente com 65 anos de idade

    Directory of Open Access Journals (Sweden)

    Ellen Simionato Valente

    2015-12-01

    Full Text Available Resumo Arterite de Takayasu é uma doença rara, de etiologia desconhecida, que acomete a aorta e seus principais ramos. É uma patologia, geograficamente mais comum no Sudeste Asiático, que acomete principalmente mulheres em idade reprodutiva. A apresentação clínica é inespecífica, com sinais e sintomas que variam de acordo com o seguimento arterial acometido. O vaso mais comumente afetado é a artéria subclávia, enquanto a estenose de artéria renal é relativamente incomum. Comprometimento cardíaco e associação com outras patologias também podem estar presentes. Apresentamos neste relato o caso de uma paciente idosa com diagnóstico tardio de arterite de Takayasu e várias comorbidades ou complicações relacionadas.

  18. A tríade “Verdadeiro-Bom-Belo”: O lugar da beleza na Idade Média

    Directory of Open Access Journals (Sweden)

    Jan A. Aertsen

    2008-06-01

    Full Text Available Neste artigo, Jan Aertsen discute a compreensão da tríade “Verdadeiro-Belo-Bom” como representante de um conjunto de questões clássicas em filosofia, a qual corresponderia, do ponto de vista moderno, à suposição de que o sujeito possui três modos distintos de se relacionar com o mundo: cognitivo, estético e prático. O autor sugere que a tríade foi formulada explicitamente pela primeira vez na Idade Média; neste período, entretanto, a beleza não era considerada um problema “estético”.

  19. A estética do corpo na filosofia e na arte da Idade Média: texto e imagem

    Directory of Open Access Journals (Sweden)

    Ricardo Luiz Silveira da Costa

    2012-01-01

    Full Text Available A ideia de beleza - e sua consequente fruição estética - variou conforme as transformações das sociedades humanas, no tempo. Durante a Idade Média, coexistiram diversas concepções de qual era o papel do corpo na hierarquia dos valores estéticos, tanto na Filosofia quanto na Arte. Nossa proposta é apresentar a estética do corpo medieval que alguns filósofos desenvolveram em seus tratados (particularmente Isidoro de Sevilha, Hildegarda de Bingen, João de Salisbury, Bernardo de Claraval e Tomás de Aquino, além de algumas representações corporais nas imagens medievais (iluminuras e esculturas, e assim analisar o tema em três vertentes: a o corpo como cárcere da alma, b o corpo como instrumento, e c o corpo como desregramento.

  20. Exigência nutricional de sódio para frangos de corte de 1 a 21 dias de idade

    OpenAIRE

    Barros José Mauricio Sthel de; Gomes Paulo Cezar; Rostagno Horacio Santiago; Albino Luiz Fernando Teixeira; Nascimento Adriana Helena do

    2001-01-01

    Com o objetivo de determinar as exigências em sódio para pintos de corte machos e fêmeas, durante a fase inicial, foram utilizados 800 pintos, sexados, da marca comercial Avian Farms, no período de 1 a 21 dias de idade, com peso médio inicial de 40,5 g, submetidos a uma dieta basal (3.000 kcal EM/kg e 21,1% de PB) deficiente em sódio (0,017%), suplementada com NaCl, correspondente aos níveis 0,077, 0,137, 0,197, 0,257 e 0,317% de sódio total. O delineamento utilizado foi o inteiramente casual...