WorldWideScience

Sample records for radiation novas rotas

  1. O PAPEL DA ÁFRICA NA NOVA ROTA DA SEDA MARÍTIMA

    Directory of Open Access Journals (Sweden)

    Diego Pautasso

    2017-01-01

    Full Text Available O objetivo do presente artigo é analisar o lugar da África na construção da Nova Rota da Seda Marítima. Este é justamente um dos vetores do ambicioso projeto chinês de integração da Ásia, Europa e África, lançada em 2013 sob título de Iniciativa OBOR (One Belt, One Road. Na medida que os desafios da reconstrução nacional são superados, a China torna-se mais assertiva e dá forma à sua estratégia de inserção mundial. Nesse sentido, a Nova Rota da Seda agrega os objetivos centrais da diplomacia da China para o século XXI, reservando à África a condição de trampolim para que o projeto se torne global.

  2. 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.

  3. 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...

  4. Testing astrophysical radiation hydrodynamics codes with hypervelocity jet experiments on the nova laser

    Energy Technology Data Exchange (ETDEWEB)

    Estabrook, K; Farley, D; Glendinning, S G; Remington, B A; Stone, J; Turner, N

    1999-09-22

    Recent shock tube experiments using the Nova laser facility have demonstrated that strong shocks and highly supersonic flows similar to those encountered in astrophysical jets can be studied in detail through carefully controlled experiment. We propose the use of high power lasers such as Nova, Omega, and NIF to perform experiments on radiation hydrodynamic problems such as jets involving the multidimensional dynamics of strong shocks. High power lasers are the only experimental facilities that can reach the very high Mach number regime. The experiments will serve both as diagnostics of astrophysically interesting gas dynamic problems, and could also form the basis of test problems for numerical algorithms for astrophysical radiation hydrodynamic codes, The potential for experimentally achieving a strongly radiative jet seems very good.

  5. Measurement of radiative proton capture on 18F and implications for oxygen-neon novae reexamined

    Science.gov (United States)

    Akers, C.; Laird, A. M.; Fulton, B. R.; Ruiz, C.; Bardayan, D. W.; Buchmann, L.; Christian, G.; Davids, B.; Erikson, L.; Fallis, J.; Hager, U.; Hutcheon, D.; Martin, L.; Murphy, A. St. J.; Nelson, K.; Ottewell, D.; Rojas, A.; Spyrou, A.

    2016-12-01

    Background: The rate of the 18F(p ,γ )19Ne reaction affects the final abundance of the radioisotope 18F ejected from novae. This nucleus is important as its abundance is thought to significantly influence the first-stage 511-keV and continuum γ -ray emission in the aftermath of novae. No successful measurement of this reaction existed prior to this work, and the rate used in stellar models had been calculated based on incomplete information from contributing resonances. Purpose: Of the two resonances thought to provide a significant contribution to the astrophysical reaction rate, located at Ec .m .=330 and 665 keV, the former has a radiative width estimated from the assumed analog state in the mirror nucleus, 19F, while the latter resonance does not have an analog state assignment, resulting in an arbitrary radiative width being assumed. As such, a direct measurement was needed to establish what role this resonance plays in the destruction of 18F at nova temperatures. This paper extends and takes the place of a previous Letter which reported the strength of the Ec .m .=665 keV resonance. Method: The DRAGON recoil separator was used to directly measure the strength of the important 665-keV resonance in this reaction, in inverse kinematics, by observing 19Ne reaction products. A radioactive 18F beam was provided by the ISAC facility at TRIUMF. R -matrix calculations were subsequently used to evaluate the significance of the results at astrophysical energies. Results: We report the direct measurement of the 18F(p ,γ )19Ne reaction with the reevaluation of several detector efficiencies and the use of an updated 19Ne level scheme in the reaction rate analysis. The strength of the 665-keV resonance (Ex=7.076 MeV) is found to be an order of magnitude weaker than currently assumed in nova models. An improved analysis of the previously reported data is presented here, resulting in a slightly different value for the resonance strength. These small changes, however, do

  6. High-energy emission from non-relativistic radiative shocks: application to gamma-ray novae

    CERN Document Server

    Vurm, Indrek

    2016-01-01

    Multiwavelength radiation from relativistic particles accelerated at shocks in novae and other astrophysical sources carries a wealth of information about the outflow properties and the microphysical processes at work near the shocks. The observation of GeV gamma-rays from novae by Fermi/LAT demonstrates that the shocks in these systems can accelerate particles to energies of at least $\\sim 10$ GeV. The low-energy extension of the same non-thermal particle distribution inevitably gives rise to emission extending into the X-ray band. Above $\\gtrsim 10$ keV this radiation can escape the system without significant absorption/attenuation, and can potentially be detected by NuSTAR. We present theoretical models for hard X-ray and gamma-ray emission from radiative shocks in both leptonic and hadronic scenarios, accounting for the rapid evolution of the downstream properties due to the fast cooling of thermal plasma. Due to strong Coulomb cooling of the mildly relativistic electrons nominally responsible for produci...

  7. CNMI Abandoned Vessel Inventory, Rota

    Data.gov (United States)

    National Oceanic and Atmospheric Administration, Department of Commerce — NOAA Abandoned Vessel Project Data for Rota. Abandoned vessels pose a significant threat to the NOAA Trust resources through physical destruction of coral habitats...

  8. 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 ...

  9. Dilemmas of a rota: Google's solution.

    Science.gov (United States)

    Qureshi, Jibran S; Javaid, Fatimah

    2015-01-01

    Doctors take many forms of leave to further career training. Many hospital rotas omit these and are not updated frequently to reflect swaps in on-call duties. As a result, confusion arises with reduced staffing levels leading to sub-optimal patient care. Using Google Sheets, rota's can be modified to be team specific, remotely accessed, and edited by any device with an internet connection and web browser. A qualitative pre and post-implementation questionnaire assessed the usefulness of the online rota. The rota was trialled on a surgical and medical team containing foundation year, core medical, core surgical, and registrar trainees. The respective surgical and medical rotas were copied, modified and pasted into a Google Sheet to contain only team specific information including all forms of leave. A link was emailed allowing teams to access and edit the rota. Post-implementation questionnaire 90% (n=10) stated they could access it remotely and 100% felt the new rota was very easy to use. Finally, 80% stated the Google Doc rota was a definite improvement on the old trust rota. The rota was then trialled on an ITU SHO rota (n=8). The results were reproducible with 88% feeling it addressed their requirements and stating it was an improvement on their old rota. As a result of the implementation appropriate staffing levels were maintained on the ward. The key advantages of the Google rota are that it included all forms of leave and helped ensure adequate staffing levels on the ward. The remote nature means easy access even if off-site and can be viewed easier on smart phones. The different privacy settings ensure security of document. The rota is updated in real-time giving an accurate representation of staffing levels - vital for service managers. The software is free to use, allowing it to work within current hospital IT framework.

  10. Novità procedurali riguardanti la Rota Romana: le facoltà speciali

    Directory of Open Access Journals (Sweden)

    Joaquín Llobell

    2013-10-01

    Full Text Available Il contributo, accettato dal Direttore, riproduce la Relazione al “V Corso di aggiornamento in diritto matrimoniale e processuale canonico” della Facoltà di Diritto Canonico della Pontificia Università della Santa Croce (Roma, 16-20 settembre 2013, ed è destinato alla pubblicazione negli Atti del Corso, per i tipi della Edusc, Roma.SOMMARIO: 1. Premessa – 2. La facoltà speciale n. I: «Le sentenze rotali che dichiarano la nullità del matrimonio siano esecutive, senza che occorra una seconda decisione conforme»: 2.1. La prima facoltà speciale vieta l’appello contro la sentenza rotale che dichiara per la prima volta la nullità del matrimonio?; 2.2. Il diritto di appello alla Rota Romana e le fattispecie in cui la Rota può emettere una prima sentenza “pro nullitate matrimonii”; 2.3. Cenni minimi sulle conseguenze della prima facoltà speciale sulla delibazione della prima sentenza a favore della nullità del matrimonio – 3. La facoltà speciale n. II: «Dinanzi alla Rota Romana non è possibile proporre ricorso per la N.C.P. [“nova causae propositio”], dopo che una delle parti ha contratto un nuovo matrimonio canonico» – 4. La facoltà speciale n. III: «Non si dà appello contro le decisioni rotali in materia di nullità di sentenze o di decreti» – 5. La facoltà speciale n. IV: «Il Decano della Rota Romana ha la potestà di dispensare per grave causa dalle Norme Rotali in materia processuale», con particolare riferimento alla modifica dei turni giudicanti per affidare le cause a collegi “videntibus septem iudicibus” – 6. La facoltà speciale n. V: «Siano avvertiti gli Avvocati Rotali circa il grave obbligo di curare con sollecitudine lo svolgimento delle cause loro affidate, sia di fiducia che d’ufficio, così che il processo davanti alla Rota Romana non ecceda la durata di un anno e mezzo» – 7. Brevissime conclusioni – Appendice (Testo delle facoltà speciali della Rota Romana, 11 febbraio 2013

  11. New routes of preparation of polyaniline films and dosimetric characterization for high-doses gamma radiation; Novas rotas de preparacao de filmes de polianilina e caracterizacao dosimetrica para radiacao gama em altas doses

    Energy Technology Data Exchange (ETDEWEB)

    Pacheco, Ana Paula Lima

    2003-08-15

    This work presents a new conducting polymeric material based on polyaniline thin films that will be used in the confection of dosimetric devices. On preparation of the films a homogeneous and viscous solution of poly (acrylic acid) and MnO{sub 2} is deposited on PMMA surface, which after dried, is immersed in an acid aniline solution. The films formed present low resistivity (6.10{sup 2} {omega}m), good mechanical resistance and adherence on the electrodes. The films were characterized by infrared spectroscopy, conductivity measurements and manganese elemental analyses. The resistance variations show linear correlation (r{sup 2} = 0,9928) with gamma irradiation dose in the range of 1000 to 6000 Gy, with medium error less than 5% and sensitivity response. The dosimetric devices present as advantage real time measurements, low cost, use in calibration of industrial radioactive sources. Moreover, this composite could in future replace Fricke dosimeter and its applications. A calibration curve is showed for PANI dosimeter, here proposed, to use at high gamma doses. (author)

  12. 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...

  13. Rota-Baxter operators on Witt and Virasoro algebras

    Science.gov (United States)

    Gao, Xu; Liu, Ming; Bai, Chengming; Jing, Naihuan

    2016-10-01

    The homogeneous Rota-Baxter operators on the Witt and Virasoro algebras are classified. As applications, the induced solutions of the classical Yang-Baxter equation and the induced pre-Lie and PostLie algebra structures are obtained.

  14. CRED REA Algal Assessment, Rota 2003 (NODC Accession 0010352)

    Data.gov (United States)

    National Oceanic and Atmospheric Administration, Department of Commerce — Twelve quadrats were sampled along 2 consecutively-placed, 25m transect lines as part of Rapid Ecological Assessments conducted at 6 sites at Rota in the...

  15. CRED REA Algal Assessments at Rota, Marianas Archipelago in 2007

    Data.gov (United States)

    National Oceanic and Atmospheric Administration, Department of Commerce — Twelve quadrats were sampled along 2 consecutively-placed, 25m transect lines, as part of Rapid Ecological Assessments, conducted at 6 sites at Rota in the Marianas...

  16. 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

  17. Rota-Baxter algebras and the Hopf algebra of renormalization

    Energy Technology Data Exchange (ETDEWEB)

    Ebrahimi-Fard, K.

    2006-06-15

    Recently, the theory of renormalization in perturbative quantum field theory underwent some exciting new developments. Kreimer discovered an organization of Feynman graphs into combinatorial Hopf algebras. The process of renormalization is captured by a factorization theorem for regularized Hopf algebra characters. Hereby the notion of Rota-Baxter algebras enters the scene. In this work we develop in detail several mathematical aspects of Rota-Baxter algebras as they appear also in other sectors closely related to perturbative renormalization, to wit, for instance multiple-zeta-values and matrix differential equations. The Rota-Baxter picture enables us to present the algebraic underpinning for the Connes-Kreimer Birkhoff decomposition in a concise way. This is achieved by establishing a general factorization theorem for filtered algebras. Which in turn follows from a new recursion formula based on the Baker-Campbell-Hausdorff formula. This allows us to generalize a classical result due to Spitzer to non-commutative Rota-Baxter algebras. The Baker-Campbell-Hausdorff based recursion turns out to be a generalization of Magnus' expansion in numerical analysis to generalized integration operators. We will exemplify these general results by establishing a simple representation of the combinatorics of renormalization in terms of triangular matrices. We thereby recover in the presence of a Rota-Baxter operator the matrix representation of the Birkhoff decomposition of Connes and Kreimer. (orig.)

  18. ``A Minority View'' Gian-Carlo Rota's Phenomenological Realism

    Science.gov (United States)

    Palombi, Fabrizio

    In 1997 Rota's second anthology was published, entitled Indiscrete Thoughts. The theses put forward in the book were "minority" positions in a Unites States cultural context that, after long having attempted to replace philosophy with logical analysis and the analysis of language (Hersh, 1997, pp. IX-X), was preparing to interpret it also in neuroscientific terms. Rota intended to show that he did not fear uncomfortable positions and chose the phrase "a minority view" as a provocative title for the philosophy section of the book, inspired by phenomenology. We cannot understand the importance of Rota's intellectual figure, within the American cultural context of the end of the twentieth century, and the importance of his heritage if we interpret it in terms of architectonic of philosophy.

  19. Experiências de rotação

    Directory of Open Access Journals (Sweden)

    W. L. Stevens

    1951-12-01

    Full Text Available Descrevemos os princípios básicos do planejamento de experiências de rotação. Apontamos a necessidade de incluir na experiência tôdas as fases das rotações em todos os anos. Mostramos o motivo por que, geralmente, não podem ser aproveitados os delieneamentos complexos desenvolvidos para experiências de um só ano. Discutimos uma experiência de rotação com milho, algodão e macuna.This paper explains the principles of planning rotation experiments. It includes a description of a rotation experiment with maize, cotton and mucuna, which is now beginning at two stations in the State of São Paulo. An account of this experiment, together with a discussion of its statistical analysis, will appear elsewhere in English.

  20. Análise de Rotas Alternativas de Transporte: O Caso da Soja de Mato Grosso

    Directory of Open Access Journals (Sweden)

    Elvio Souza Resende

    2011-06-01

    Full Text Available Normal 0 21 false false false PT-BR X-NONE X-NONE A proposta deste trabalho é analisar as rotas de transporte de soja do Estado de Mato Grosso. O sistema de transporte da soja C um ponto importante na cadeia produtiva, pois a maior parte dos custos desta commodity é dado pelos custos de transporte. Nesse sentido, a otimização desse segmento é essencial para aumentar a competitividade da soja mato-grossense no mercado internacional. O complexo soja brasileiro tem aumentado a sua participação nas exportações dos produtos agrícolas nos últimos dez anos, mas os investimentos de outros países fazem com que as exportações brasileiras não fiquem tocadas apenas no crescimento da produção mas sim na eficiência de toda a cadeia produtiva. Levando em consideração os investimentos previstos do PAC (Plano de Aceleração do Crescimento em infraestrutura para Mato Grosso procurou-se estabelecer novas rotas para o escoamento da produção de soja em Mato Grosso. Assim concluiu-se que a expansão da ferrovia ate Rondonópolis, a recuperação e pavimentação da BR-163 proporcionarão condições para a redução do custo do frete para a soja mato-grossense.

  1. O feminismo em novas rotas e visões Feminism on new routes and views

    Directory of Open Access Journals (Sweden)

    Matilde Ribeiro

    2006-12-01

    Full Text Available O presente texto se baseia no debate proposto por Mary Hawkesworth no artigo "A semiótica de um encontro prematuro: o feminismo em uma era pós-feminista", orientando-se por um olhar latino-americano-caribenho sobre as transformações do feminismo e as conquistas das mulheres em momentos cruciais dessa articulação, relembrando fases memoráveis como a renovação dos ideais feministas, a autonomia do movimento de mulheres negras e sua inter-relação com o ativismo negro e feminista, articulações internacionais sintonizados com a realidade/diversidade brasileira e a incorporação da agenda feminista nas instâncias governamentais. A autora expõe o dinamismo e a capacidade de retroalimentação do feminismo brasileiro, características que possibilitam a força necessária para sua sobrevivência e inovações harmonizadas com a evolução de valores sociais diante das conquistas decorrentes de sua existência nos cenários local, regional e global. Substancialmente, desenvolve o texto com ênfase no ativismo local como desencadeador de uma ação efetiva de Estado para eqüidade de gênero e raça.This paper is based on the debate proposed by Mary Hawkesworth in "The semiotics of a Premature Burial: Feminism in a Post-Feminist Age". It is guided by a Latin-American and Caribbean view of the transformations of feminism and of women's achievements in critical moments of that articulation, recollecting outstanding periods such as the renovation of feminist ideals; the autonomy of the black women's movement and its inter-relation with black and feminist activism; and international articulations tuned with Brazilian reality/diversity and with the incorporation of the feminist agenda within governmental instances. The author portrays how the verve and retro-feeding capacity of Brazilian feminism provide the necessary strength for its survival, as well as for its innovations which are consonant with the evolution of social values, leading to its various achievements as they stem from local, regional and global arenas. Substantially, the author has developed this text with a sharp focus on local activism as the trigger for effective governmental action towards achieving gender and race equity.

  2. 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.

  3. The Star and the Whole Gian-Carlo Rota on Mathematics and Phenomenology

    CERN Document Server

    Palombi, Fabrizio

    2011-01-01

    The Star and the Whole: Gian-Carlo Rota on Mathematics and Phenomenology, authored by Fabrizio Palombi, is the first book to study Rota's philosophical reflection. Rota (1932--1999) was a leading figure in contemporary mathematics and an outstanding philosopher, inspired by phenomenology, who made fundamental contributions to combinatorial analysis, and trained several generations of mathematicians in his long career at the Massachusetts Institute of Technology (MIT) and the Los Alamos National Laboratory. The first chapter of the book reconstructs Rota's cultural biography and examines his ph

  4. 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.

  5. Measurement of radiative proton capture on F18 and implications for oxygen-neon novae reexamined

    Energy Technology Data Exchange (ETDEWEB)

    Akers, C.; Laird, A. M.; Fulton, B. R.; Ruiz, C.; Bardayan, D. W.; Buchmann, L.; Christian, G.; Davids, B.; Erikson, L.; Fallis, J.; Hager, U.; Hutcheon, D.; Martin, L.; Murphy, A. St. J.; Nelson, K.; Ottewell, D.; Rojas, A.; Spyrou, A.

    2016-12-15

    The rate of the F-18(p, gamma)Ne-19 reaction affects the final abundance of the gamma-ray observable radioisotope F-18, produced in novae. However, no successful measurement of this reaction exists and the rate used is calculated from incomplete information on the contributing resonances. Of the two resonances thought to play a significant role, one has a radiative width estimated from the assumed analogue state in the mirror nucleus, F-19. The second does not have an analogue state assignment at all, resulting in an arbitrary radiative width being assumed. Here, we report the first successful direct measurement of the F-18(p, gamma)Ne-19 reaction. The strength of the 665 keV resonance (E-x = 7.076 MeV) is found to be over an order of magnitude weaker than currently assumed in nova models. Reaction rate calculations show that this resonance therefore plays no significant role in the destruction of F-18 at any astrophysical energy.

  6. Rota do Tropeiro: a cultural entertainment game for Android platform

    Directory of Open Access Journals (Sweden)

    Estevan Strapazzon Ruschel

    2016-06-01

    Full Text Available This paper presents a cultural entertainment game entitled “Rota do Tropeiro”. The aim of our article is to briefly present well-known tools that can be integrated and used by beginners to develop games with quality and optimized performance, especially for the Android platform. The document describes our game prototype, showing techniques and methodologies applied and highlighting new challenges. As a result, we produced a mobile game for end-users, and creative stuffs like animations, geometric models and artificial intelligence scripts.

  7. Quasi-idempotent Rota-Baxter operators arising from quasi-idempotent elements

    Science.gov (United States)

    Jian, Run-Qiang

    2017-02-01

    In this short note, we construct quasi-idempotent Rota-Baxter operators by quasi-idempotent elements and show that every finite dimensional Hopf algebra admits nontrivial Rota-Baxter algebra structures and tridendriform algebra structures. Several concrete examples are provided, including finite quantum groups and Iwahori-Hecke algebras.

  8. Data of evolutionary structure change: 1CSKA-2ROTA [Confc[Archive

    Lifescience Database Archive (English)

    Full Text Available 1CSKA-2ROTA 1CSK 2ROT A A -----GTECIAKYNFHGTAEQDLPFCKGDVLTIVAVTKD... 2ROT A 2ROTA LTLLN-S... -53.63399887084961 -11.517000198364258 tion> 0.460999995470047 -0.061000000685453415 tion> 2.0833489894866943 3.118304967880249 ...

  9. Data of evolutionary structure change: 1CSKD-2ROTA [Confc[Archive

    Lifescience Database Archive (English)

    Full Text Available 1CSKD-2ROTA 1CSK 2ROT D A -----GTECIAKYNFHGTAEQDLPFCKGDVLTIVAVTKD... 2ROT A 2ROTA TLLNS-...3799819946289 -33.77199935913086 -31.43400001525879 tion> 0.8009999990...4 0.15399999916553497 tion> 1.8454389572143555 3.4630019664764404 ...

  10. Data of evolutionary structure change: 1CSKB-2ROTA [Confc[Archive

    Lifescience Database Archive (English)

    Full Text Available 1CSKB-2ROTA 1CSK 2ROT B A -----GTECIAKYNFHGTAEQDLPFCKGDVLTIVAVTKD...x> 2ROT A 2ROTA TLLN...3 -58.54800033569336 -12.753000259399414 tion> -0.21899999678134918 -0.16899999976158142 tion> 1.8727550506591797 3.4557619094848633 ...

  11. Data of evolutionary structure change: 1CSKC-2ROTA [Confc[Archive

    Lifescience Database Archive (English)

    Full Text Available 1CSKC-2ROTA 1CSK 2ROT C A -----GTECIAKYNFHGTAEQDLPFCKGDVLTIVAVTKD...entryChain> 2ROT A 2ROTA TLLNS-TN...0045776367 -65.2699966430664 -31.405000686645508 tion> -0.953000009059...5596 -0.2290000021457672 tion> 1.8559880256652832 3.4498000144958496 ...

  12. 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.

  13. 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.

  14. Tres mujeres diferentes La mujer rota Simone de Beauvoir

    OpenAIRE

    Cárdenas González, Alejandra

    2012-01-01

    llegaba con el libro en mente, lo pedía y adiós. Pero ese día me topé con La mujer rota de Simone de Beauvoir. Reconocía a la autora por mi último año de  colegio, cuando guiada por mi querida maestra de español, recordaba a su amante más intenso Jean Paul Sartre y a uno de sus colegas Albert Camus; además sabía el nombre de sus libros más conocidos pero nunca me había metido de lleno a su lectura. Allí estaba en la biblioteca, debatiéndome entre El Decamerón de Bocaccio y La peste de Ca...

  15. 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...

  16. Comparative evaluation of coagglutination and latex agglutination test (Rotalex kit for detection of rota virus.

    Directory of Open Access Journals (Sweden)

    Mathur M

    1993-07-01

    Full Text Available Coagglutination test was compared with commercially available latex agglutination test (Rotalex kit for detection of rota virus in faecal samples from clinically suspected cases of viral gastroenteritis. Out of 80 test samples 16 (20% and 20 (25.3% were positive for rota virus antigen by Rotalex kit and coagglutination test respectively. All the 40 controls were negative for viral antigen by Rotalex kit and only one gave positive result by coagglutination test. Coagglutination test was found to be economical, sensitive and specific for screening and rapid diagnosis of Rota virus diarrhoea.

  17. Rota-Baxter Algebras on Quasi Hopf Module Algebras%拟Hopf-模上的Rota-Baxter代数

    Institute of Scientific and Technical Information of China (English)

    程腾; 王顶国; 程诚

    2014-01-01

    Let H be a Hopf algebra,the main aim of this paper is to extend the theorem of Hopf(co) quasigroup.Let H be a Hopf quasigroup and (M,φ)be an right quasi H-Hopf module algebra,then (M, P )is a Rata-Baxter algebra of weight-1 .%把 Run-qiang Jian文中的H 为 Hopf代数的情况推广到H 为 Hopf(余)拟群,其主要结论:设H是 Hopf拟群,(M,φ)是一右拟H-Hopf模代数,则(M,P)是权为-1的 Rota-Baxter代数。

  18. Folha rota, de Machado de Assis: mulheres livres e pobres na ordem patriarcal

    National Research Council Canada - National Science Library

    da Conceicao Silva, Eliane

    2009-01-01

    Este artigo analisa o conto Folha rota (1878), de Machado de Assis, levando-se em conta o processo de transformacao do patriarcalismo, haja vista sua decadencia no contexto de crescente urbanizacao durante o seculo XIX...

  19. CRED REA Fish Team Stationary Point Count Surveys at Rota, Marianas Archipelago, 2005

    Data.gov (United States)

    National Oceanic and Atmospheric Administration, Department of Commerce — Stationary Point Counts at 4 stations at each survey site were surveyed as part of Rapid Ecological Assessments (REA) conducted at 6 sites around Rota in the...

  20. CRED REA Fish Team Belt Transect Survey at Rota, Marianas Archipelago, 2005

    Data.gov (United States)

    National Oceanic and Atmospheric Administration, Department of Commerce — Belt transects along 3 consecutively-placed, 25m transect lines were surveyed as part of Rapid Ecological Assessments conducted at 6 sites at Rota in the Marianas...

  1. CRED REA Fish Team Stationary Point Count Surveys at Rota Island, 2003

    Data.gov (United States)

    National Oceanic and Atmospheric Administration, Department of Commerce — Stationary Point Counts at 4 stations at each survey site were surveyed as part of Rapid Ecological Assessments conducted at 6 sites at Rota Island in the...

  2. From combinatorics to philosophy the legacy of G.-C. Rota

    CERN Document Server

    Damiani, Ernesto; Marra, Vincenzo

    2009-01-01

    This book provides an assessment of G. -C. Rota's legacy to international research in mathematics, philosophy and computer science. It includes chapters by leading researchers as well as a number of invited research papers.

  3. CRED REA Algal Assessments at Rota Island, Marianas Archipelago in 2005

    Data.gov (United States)

    National Oceanic and Atmospheric Administration, Department of Commerce — As part of Rapid Ecological Assessments (REA), Twelve quadrats were sampled along 2 consecutively-placed, 25m transect lines, conducted at 6 sites at Rota Island in...

  4. O DESENVOLVIMENTO DO TURISMO: A Rota Colonial Baumschneis em Dois Irmãos/RS

    Directory of Open Access Journals (Sweden)

    Mary Sandra Guerra Ashton

    2011-11-01

    Full Text Available Resumo: Esse trabalho analisa a Rota Colonial Baumschneis, localizada em Dois Irmãos/RS, com o objetivo de investigar a sua contribuição para o desenvolvimento do turismo no município. Pretende revelar a importância da Rota e seu papel no desenvolvimento do turismo municipal. O método utilizado foi o exploratório, com revisão bibliográfica e pesquisa de campo na Rota Colonial. Os resultados mostram o perfil dos proprietários e traçam o histórico do projeto. Palavras-chave: Turismo. Desenvolvimento do Turismo. Rota Colonial Baumschneis. Dois Irmãos/RS

  5. CRED REA Fish Team Stationary Point Count Surveys at Rota, Marianas Archipelago (MA) in 2007

    Data.gov (United States)

    National Oceanic and Atmospheric Administration, Department of Commerce — Stationary Point Counts at 4 stations at each survey site were surveyed as part of Rapid Ecological Assessments (REA) conducted at 6 sites around Rota in the...

  6. CRED REA Fish Team Belt Transect Survey at Rota Island, 2003

    Data.gov (United States)

    National Oceanic and Atmospheric Administration, Department of Commerce — Belt transects along 3 consecutively-placed, 25m transect lines were surveyed as part of Rapid Ecological Assessments conducted at 6 sites at Rota in the...

  7. Gridded multibeam bathymetry of Rota Island, Commonwealth of the Northern Mariana Islands (CNMI)

    Data.gov (United States)

    National Oceanic and Atmospheric Administration, Department of Commerce — Gridded bathymetry shelf, bank and slope environments of Rota Island, CNMI. Bottom coverage was achieved in depths between 0 and -1905 meters. The netCDF and Arc...

  8. OPUS-Rota: a fast and accurate method for side-chain modeling.

    Science.gov (United States)

    Lu, Mingyang; Dousis, Athanasios D; Ma, Jianpeng

    2008-09-01

    In this paper, we introduce a fast and accurate side-chain modeling method, named OPUS-Rota. In a benchmark comparison with the methods SCWRL, NCN, LGA, SPRUCE, Rosetta, and SCAP, OPUS-Rota is shown to be much faster than all the methods except SCWRL, which is comparably fast. In terms of overall chi (1) and chi (1+2) accuracies, however, OPUS-Rota is 5.4 and 8.8 percentage points better, respectively, than SCWRL. Compared with NCN, which has the best accuracy in the literature, OPUS-Rota is 1.6 percentage points better for overall chi (1+2) but 0.3 percentage points weaker for overall chi (1). Hence, our algorithm is much more accurate than SCWRL with similar execution speed, and it has accuracy comparable to or better than the most accurate methods in the literature, but with a runtime that is one or two orders of magnitude shorter. In addition, OPUS-Rota consistently outperforms SCWRL on the Wallner and Elofsson homology-modeling benchmark set when the sequence identity is greater than 40%. We hope that OPUS-Rota will contribute to high-accuracy structure refinement, and the computer program is freely available for academic users.

  9. New Novae snack point

    CERN Multimedia

    2012-01-01

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

  10. Aprendizagens e novas tecnologias

    Directory of Open Access Journals (Sweden)

    Pedro Demo*

    2011-06-01

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

  11. Medical rota changes and venous thromboembolism prophylaxis in orthopaedic patients.

    Science.gov (United States)

    Bohler, Iain; George Mackenzie Jardine, Alan

    2014-01-01

    Efficacy of clinical guidelines to improve patient care is highly dependent on the ability of hospital teams to interpret and implement advised standards of care. Trimester and bi-annual rotation changes often see transference and loss of acquired experience and knowledge from wards with ensuing shortfalls in patient safety and care quality. Such shortfalls were noticed in the ability of our unit to adhere to national venous thromboembolism (VTE) prophylaxis measures. A prospective quality improvement audit was embarked upon to address this. An initial audit of VTE prophylaxis in 112 patients demonstrated just 71% compliance with suggested measures. Errors were predominantly medical in origin and secondary to poor understanding, interpretation, and knowledge of VTE guidelines. Errors were also noted in nursing and patient compliance to measures. Repeated re-auditing demonstrated increased error (following initial improvement post audit) after periods of medical staff rotation. Through education of junior medical and nursing staff, and of patients, the unit was able to achieve 100% compliance. Rota changes often induce conflict of interest between maintaining adequate services and high levels of patient care or providing suitable and informed induction programmes for new medical staff. Emphasised education of VTE prophylaxis guidelines has now become part of induction of junior medical staff, whilst ward based measures ensure daily compliance. The success of the audit strategy has led to its use throughout other surgical units within the hospital.

  12. 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.

  13. The Galactic Nova Rate Revisited

    CERN Document Server

    Shafter, A W

    2016-01-01

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

  14. 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 ...

  15. Population trends of Mariana Crow Corvus kubaryi on Rota, Commonwealth of the Northern Mariana Islands

    Science.gov (United States)

    Plentovich, S.; Morton, J.M.; Bart, J.; Camp, R.J.; Lusk, M.; Johnson, N.; VanderWerf, E.

    2005-01-01

    Endemic to the islands of Guam and Rota in the Mariana Islands, Mariana Crow Corvus kubaryi is the only corvid in Micronesia. Currently, it survives on Guam only because of translocation of individuals from Rota (1999-2003). Island-wide surveys in 1982 and 1995 on Rota yielded population estimates of 1,348 and 592 respectively, indicating a 56% decrease in only 13 years. A sharp decline in the only viable Mariana Crow population has serious implications for conservation efforts on Rota and for efforts to re-establish the Guam population. However, the validity of the apparent decline has been debated among scientists and government management agencies. We augmented the 1982 and 1995 island-wide VCP surveys with (1) an additional island-wide survey conducted in 1998, and (2) roadside surveys conducted during 1991-1993 and again during 1999-2002. We also outline historical changes in Rota's limestone forest based on aerial photographs and historical information. Data from all surveys indicate a significant decline in the Mariana Crow population. Declines occurred especially along the north-central coast and in the area east of the airport known as As Dudo in the 1990s, but the data indicate an island-wide decline over the entire span of the surveys. introduced predators, human persecution, and habitat loss and degradation by anthropogenic and natural causes have all contributed to the decline. Long-term preservation of this species will require effective brown treesnake Boiga irregularis control, habitat protection, continued monitoring and research, and increased public education and awareness of Rota's rare and endangered species. ?? BirdLife International 2005.

  16. 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.

  17. 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...

  18. Recurrent Novae in M31

    CERN Document Server

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

    2014-01-01

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

  19. Franchising in Nova Scotia

    Energy Technology Data Exchange (ETDEWEB)

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

    1998-09-01

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

  20. Terra Nova update

    Energy Technology Data Exchange (ETDEWEB)

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

    2002-07-01

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

  1. Nova Mus 2008 = QY Mus

    Science.gov (United States)

    Templeton, Matthew R.

    2008-10-01

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

  2. 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.

  3. The potential for typhoon impact on bird populations on the island of Rota, Northern Mariana

    Directory of Open Access Journals (Sweden)

    Ha, C.

    2012-12-01

    Full Text Available Numerous independent analyses of climate change have suggested that changing weather patterns are resulting in increasing frequency or intensity of hurricanes and typhoons. We explore the relationship between cyclonic event frequency and severity on measures of bird abundance on the island of Rota, in the Northern Mariana Islands to determine if changes in cyclonic event pattern might be related to the local decline of avian species. We developed a database of Rota cyclonic event encounters since 1952 and three primary variables for analysis of cyclonic event behavior were then derived from this data: Time-Between-Typhoon-Encounters, Distance from Rota at closest approach, and Pressure at the center of the cyclonic event at the point of closest approach Three similar smoothed variables were derived relative to each Breeding Bird and Variable Circle Plot census time point. Multivariate general linear models were constructed separately for each bird abundance data set with multiple species as dependent variables and smoothed cyclonic event time-between-encounter, distance-at-closest- point, and central-pressure-at-closest-point as independent variables. Cyclonic event behavior in relation to Rota did not exhibit an increase in frequency, as sometimes perceived, but did show a significant decrease in distance to the island and an increase in intensity as measured by central pressure. Several species abundances showed significant relationships with cyclonic event pressure or distance, including the Mariana Crow, Philippine Turtle Dove, and Rufous Fantail. It appears that changes in cyclonic event “behavior” could be impacting forest-bird populations on Rota. Overall, bird population declines may be due to a combined effect of habitat loss, introduced species pressure, and cyclonic events, where any one of the factors might be enough to tip a species into decline.

  4. RECURRENT NOVAE IN M31

    Energy Technology Data Exchange (ETDEWEB)

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

    2015-02-01

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

  5. 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.

  6. 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.

  7. 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.

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

    CERN Document Server

    van Rossum, Daniel R

    2012-01-01

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

  9. 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

  10. Experiências em Nova Iorque na década de 1970

    Directory of Open Access Journals (Sweden)

    Dária Jaremtchuk

    2008-12-01

    Full Text Available Este artigo discute a presença de dois artistas brasileiros em Nova Iorque na década de 1970, bem como suas possíveis conexões com aquele circuito de arte. Também são relacionados os interesses econômicos e diplomáticos que contribuíram para que os Estados Unidos se tornassem uma rota alternativa para os artistas brasileiros que se exilavam, voluntariamente ou não, nas décadas de 1960 e 1970.This article discusses about two brazilian artists in New York in 1970, as well as their conexions with the circuit of art. Additionally, this is also related to the economic interest and diplomats wich contributed to making the United States as an alternative route for the contemporary artists who left Brazil, voluntarily or not,in the decades of the 60's and 70's.

  11. 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...

  12. C-CAP Commonwealth of the Northern Mariana Islands (CNMI), Rota 1946-2005-Era Land Cover Change Analysis

    Data.gov (United States)

    National Oceanic and Atmospheric Administration, Department of Commerce — This data set contains the 1946-era and 2005-era classifications of Rota, Commonwealth of the Northern Mariana Islands and can be used to analyze change. This data...

  13. Hopf algebras of rooted forests, cocyles, and free Rota-Baxter algebras

    Science.gov (United States)

    Zhang, Tianjie; Gao, Xing; Guo, Li

    2016-10-01

    The Hopf algebra and the Rota-Baxter algebra are the two algebraic structures underlying the algebraic approach of Connes and Kreimer to renormalization of perturbative quantum field theory. In particular, the Hopf algebra of rooted trees serves as the "baby model" of Feynman graphs in their approach and can be characterized by certain universal properties involving a Hochschild 1-cocycle. Decorated rooted trees have also been applied to study Feynman graphs. We will continue the study of universal properties of various spaces of decorated rooted trees with such a 1-cocycle, leading to the concept of a cocycle Hopf algebra. We further apply the universal properties to equip a free Rota-Baxter algebra with the structure of a cocycle Hopf algebra.

  14. Marketing plan for online aqctivity of Rota Vicentina boosting direct website sales

    OpenAIRE

    2016-01-01

    The nature tourism experienced a great expansion of its market with the appearance of different lifestyles. In this Work Project a study regarding the website direct sales of Rota Vicentina was developed. Its website shows the idea of being solely an information structure and not a purchase one, leading to a current absence of online sales. Hence, it is suggested the modification of its business model, using different instruments and channels. Some digital marketing recommen...

  15. Looking for Larvae Above an Erupting Submarine Volcano, NW Rota-1, Mariana Arc

    Science.gov (United States)

    Hanson, M.; Beaulieu, S.; Tunnicliffe, V.; Chadwick, W.; Breuer, E. R.

    2015-12-01

    In 2009 the first marine protected areas for deep-sea hydrothermal vents in U.S. waters were established as part of the Volcanic Unit of the Marianas Trench Marine National Monument. In this region, hydrothermal vents are located along the Mariana Arc and back-arc spreading center. In particular hydrothermal vents are located near the summit of NW Rota-1, an active submarine volcano on the Mariana Arc which was erupting between 2003 through 2010 and ceased as of 2014. In late 2009, NW Rota-1 experienced a massive landslide decimating the habitat on the southern side of the volcano. This presented an enormous natural disturbance to the community. This project looked at zooplankton tow samples taken from the water column above NW Rota-1 in 2010, searching specifically for larvae which have the potential to recolonize the sea floor after such a major disturbance. We focused on samples for which profiles with a MAPR sensor indicated hydrothermal plumes in the water column. Samples were sorted in entirety into coarse taxa, and then larvae were removed for DNA barcoding. Overall zooplankton composition was dominated by copepods, ostracods, and chaetognaths, the majority of which are pelagic organisms. Comparatively few larvae of benthic invertebrates were found, but shrimp, gastropod, barnacle, and polychaete larvae did appear in low numbers in the samples. Species-level identification obtained via genetic barcoding will allow for these larvae to be matched to species known to inhabit the benthic communities at NW Rota-1. Identified larvae will give insight into the organisms which can re-colonize the seafloor vent communities after a disturbance such as the 2009 landslide. Communities at hydrothermal vents at other submarine volcanoes in the Monument also can act as sources for these planktonic, recolonizing larvae. As the microinvertebrate biodiversity in the Monument has yet to be fully characterized, our project also provides an opportunity to better describe both

  16. Acerca del hormigón de la Base de Rota

    Directory of Open Access Journals (Sweden)

    López Ruiz, Álvaro

    1963-09-01

    Full Text Available Not availableCon reconocimiento a las entidades Thompson & Lichtner Co. Inc., Brown-Raymond-Walsh y O. I. C. C, supervisares del Laboratorio de ensayo y proyecto de materiales de construcción de la Base de Rota, en el cual el autor trabajó como "Senior testing engineer", por las facilidades dadas para la realización de este trabajo.

  17. 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?

  18. 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....

  19. 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....

  20. 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 ...

  1. Rotas de processo para minérios goethíticos

    OpenAIRE

    Aloisio Sa Cabral

    2010-01-01

    O estudo proposto tem por objetivo desenvolver uma rota de processo para beneficiar um corpo de minério de ferro com previsão de 14 anos de operação. O empreendimento está localizado no estado de Minas Gerais, aproximadamente 40km a sudeste de Belo Horizonte. Ocupará uma área aproximada de 1.600 hectares, situada parcialmente nos municípios de Rio Acima, Raposos, Caeté e Santa Bárbara, sendo a empresa empreendedora a Vale. O corpo de minério estudado foi denominado de ROM goethítico rico e po...

  2. 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.

  3. Produtividade do algodoeiro herbáceo em plantio direto no Cerrado com rotação de culturas

    Directory of Open Access Journals (Sweden)

    Corrêa José Carlos

    2004-01-01

    Full Text Available O experimento, instalado em um Latossolo Vermelho-Amarelo muito argiloso, teve o objetivo de avaliar o efeito da rotação de culturas na produtividade do algodoeiro herbáceo (Gossypium hirsutum L. r. latifolium Hutch em plantio direto sob condições de sequeiro no Cerrado. O delineamento experimental foi de blocos casualizados com cinco tratamentos e quatro repetições. Os tratamentos consistiram das rotações soja-milheto-soja-milheto-algodoeiro; soja-amaranto-soja-nabo forrageiro-soja-algodoeiro; soja-sorgo granífero-soja-sorgo granífero-algodoeiro; soja-aveia preta-soja-aveia preta-algodoeiro e soja-soja-algodoeiro. A maior produtividade do algodoeiro foi obtida com a rotação de soja e milheto, em que houve melhor controle de plantas daninhas.

  4. 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...

  5. Representações sociais de caminhoneiros de rota curta sobre HIV/AIDS

    Directory of Open Access Journals (Sweden)

    Laio Magno Santos de Sousa

    2014-08-01

    Full Text Available Neste estudo qualitativo objetivou-se analisar representações sociais de caminhoneiros de rota curta sobre a AIDS, transmissão do HIV e prevenção da AIDS. Envolveu 19 caminhoneiros de rota curta, de uma associação em Vitória da Conquista-BA. A produção dos dados foi por intermédio de entrevista semiestruturada e por análise de conteúdo temática, sendo identificadas três categorias êmicas. Os resultados mostraram que as representações sociais da AIDS estavam ancoradas nos constructos: "doença ruim", "doença perigosa", "doença incurável" e "doença que mata". A transmissão do HIV relacionou-se ao sexo desprotegido com profissionais do sexo, gays e contato com sangue contaminado; a prevenção da AIDS foi representada pelo uso da camisinha nas relações extraconjugais e pela fidelidade da esposa. Apreendeu-se que as representações sobre AIDS estão embasadas em conhecimentos do início da epidemia e fundamentadas no distanciamento dos indivíduos, configurando quadro importante para a reflexão sobre o processo de vulnerabilização.

  6. 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.

  7. 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 ...

  8. 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.

  9. 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.

  10. 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.

  11. 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.

  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. Predicting a Luminous Red Nova

    Science.gov (United States)

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

    2016-05-01

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

  14. A transitoriedade: uma nova leitura

    Directory of Open Access Journals (Sweden)

    José Otávio de Vasconcellos Naves

    2008-12-01

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

  15. 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...

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

    CERN Document Server

    Vlasov, Andrey Dmitrievich; Metzger, Brian David

    2016-01-01

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

  17. 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.

  18. Glutathione Transferase as a Potential Marker for Gut Epithelial Injury versus the Protective Role of Breast Milk sIgA in Infants with Rota Virus Gastroenteritis

    Directory of Open Access Journals (Sweden)

    Lobna S. Sherif

    2015-11-01

    CONCLUSION: Breast feeding should be encouraged and highly recommended in the first two years of life as it provides Secretory IgA to breast fed infants who in turn protect them against epithelial damage caused by Rota viral gastroenteritis.

  19. Evaluation of an open-rota system in a Danish psychiatric hospital: a mechanism for improving job satisfaction and work-life balance.

    Science.gov (United States)

    Pryce, Joanna; Albertsen, Karen; Nielsen, Karina

    2006-05-01

    To evaluate the impact of an open-rota scheduling system on the health, work-life balance and job satisfaction of nurses working in a psychiatric ward in Denmark. The effects of shift rotation and scheduling are well known; however, little is known about the wider benefits of open-rota systems. Method A structured questionnaire was distributed to control and intervention groups preintervention and postintervention (20 months). Nurses within the intervention group trialed an open-rota system in which nurses designed their own work-rest schedules. Nurses in the intervention group reported that they were more satisfied with their work hours, less likely to swap their shift when working within the open-rota system and reported significant increases in work-life balance, job satisfaction, social support and community spirit when compared with nurses in the control groups. The ownership and choice over work-rest schedules has benefits for nurses, and potentially the hospital.

  20. 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

  1. 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...

  2. 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.

  3. Propriedades do solo e sistema radicular do feijoeiro irrigado em rotação de culturas

    Directory of Open Access Journals (Sweden)

    E. B. Wutke

    2000-09-01

    Full Text Available O crescimento do sistema radicular do feijoeiro irrigado, cultivar IAC-Carioca, sob pivô central, em rotação com pousio, milho, aveia preta, Crotalaria juncea L., guandu (Cajanus cajan (L. Millsp. e mucuna preta (Mucuna aterrima, no período não-convencional de cultivo no outono-inverno, foi avaliado de 1993 a 1995, em Latossolo Vermelho eutroférrico típico, em área experimental do Instituto Agronômico, em Ribeirão Preto, São Paulo. A rotação de culturas do feijoeiro com milho e adubos verdes favoreceu a redução da resistência do solo à penetração na camada arável, garantiu a manutenção do teor de matéria orgânica do solo, bem como possibilitou a redução da acidez e o aumento do índice de saturação por bases (V% em profundidade em relação ao teor inicial. A velocidade de infiltração básica da água no solo foi favorecida pela inclusão da mucuna preta, da Crotalaria juncea L. e do milho, no esquema de rotações. A profundidade efetiva observada do seu sistema radicular foi de 0,35 a 0,40 m.

  4. The 2010 nova outburst of the symbiotic Mira V407 Cyg

    CERN Document Server

    Munari, U; Ashok, N M; Banerjee, D P K; Valisa, P; Milani, A; Siviero, A; Dallaporta, S; Castellani, F

    2010-01-01

    The nova outburst experienced in 2010 by the symbiotic binary Mira V407 Cyg has been extensively studied at optical and infrared wavelengths with both photometric and spectroscopic observations. This outburst, reminiscent of similar events displayed by RS Oph, can be described as a very fast He/N nova erupting while being deeply embedded in the dense wind of its cool giant companion. The hard radiation from the initial thermonuclear flash ionizes and excites the wind of the Mira over great distances (recombination is observed on a time scale of 4 days). The nova ejecta is found to progressively decelerate with time as it expands into the Mira wind. This is deduced from line widths which change from a FWHM of 2760 km/s on day +2.3 to 200 km/s on day +196. The wind of the Mira is massive and extended enough for an outer neutral and unperturbed region to survive at all outburst phases.

  5. 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.

  6. 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.

  7. ROTA DE PROCESSO PARA CONCENTRAÇÃO DE MINÉRIOS DE FERRO HIDRATADOS

    Directory of Open Access Journals (Sweden)

    Gunter Chaves Lipper

    2014-07-01

    Full Text Available Este trabalho tem como objetivo desenvolver uma rota de processo para reduzir a influência negativa dos minérios hidratados, principalmente os goethíticos, na qualidade do concentrado de minério de ferro de alto teor. Foi comprovado que o circuito convencional de flotação deve ser dividido em grossos e finos, com esta divisão espera-se um ganho de 2% na recuperação mássica no concentrado final sem perda de qualidade. Além da amostra de concentrado da primeira etapa de obtenção de pellet feed, foram testadas outras amostras com níveis diferentes de hidratação em pH 7, utilizando-se sulfato de sódio como ativador de superfície da hematita, aquecimento da polpa em 85ºC para diminuir a tensão superficial e melhorar a estabilidade de bolhas e também foi testada a utilização de ultrassom para expulsão das partículas ultrafinas dos interstícios das partículas maiores e porosas. Foi então demonstrado que é possível flotar hematita e aumentar o teor de ferro no concentrado final em 0,5%.

  8. 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 ...

  9. 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...

  10. Current land bird distribution and trends in population abundance between 1982 and 2012 on Rota, Mariana Islands

    Science.gov (United States)

    Camp, Richard J.; Brinck, Kevin W.; Gorresen, P. Marcos; Amidon, Fred A.; Radley, Paul M.; Berkowitz, S. Paul; Banko, Paul C.

    2015-01-01

    The western Pacific island of Rota is the fourth largest human-inhabited island in the Mariana archipelago and designated an Endemic Bird Area. Between 1982 and 2012, 12 point-transect distance-sampling surveys were conducted to assess bird population status. Surveys did not consistently sample the entire island; thus, we used a ratio estimator to estimate bird abundances in strata not sampled during every survey. Trends in population size were reliably estimated for 11 of 13 bird species, and 7 species declined over the 30-y time series, including the island collared-dove Streptopelia bitorquata, white-throated ground-dove Gallicolumba xanthonura, Mariana fruit-dove Ptilinopus roseicapilla, collared kingfisher Todiramphus chloris orii, Micronesian myzomela Myzomela rubratra, black drongo Dicrurus macrocercus, and Mariana crow Corvus kubaryi. The endangered Mariana crow (x̄  =  81 birds, 95% CI 30–202) declined sharply to fewer than 200 individuals in 2012, down from 1,491 birds in 1982 (95% CI  =  815–3,115). Trends increased for white tern Gygis alba, rufous fantail Rhipidura rufifrons mariae, and Micronesian starling Aplonis opaca. Numbers of the endangered Rota white-eye Zosterops rotensis declined from 1982 to the late 1990s but returned to 1980s levels by 2012, resulting in an overall stable trend. Trends for the yellow bittern Ixobrychus sinensis were inconclusive. Eurasian tree sparrow Passer montanus trends were not assessed; however, their numbers in 1982 and 2012 were similar. Occupancy models of the 2012 survey data revealed general patterns of land cover use and detectability among 12 species that could be reliably modeled. Occupancy was not assessed for the Eurasian tree sparrow because of insufficient detections. Based on the 2012 survey, bird distribution and abundance across Rota revealed three general patterns: 1) range restriction, including Mariana crow, Rota white-eye, and Eurasian tree sparrow; 2) widespread distribution, low

  11. 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

  12. 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.

  13. Aspectos teóricos e computacionais na resolução do problema de rotas e cobertura multiveículo : Theoretical and computational aspects of multivehicle covering tour problem's resolution

    OpenAIRE

    Rodolfo Cunha Oliveira

    2015-01-01

    Nesta dissertação, estudamos os aspectos teóricos e computacionais para o Problema de Rotas de Cobertura Multiveículo ($m$-PRC). Neste problema, alguns vértices devem pertencer a uma rota, enquanto outros devem ficar suficientemente próximos das rotas ótimas. A adaptação do problema sugerida por W. Oliveira et al. (2014) é considerada neste trabalho. Nela, a quantidade de vértices pertencentes as diferentes rotas deve ser equilibrada, com o objetivo de estudar um importante aspecto do problem...

  14. 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.

  15. 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.

  16. Curva de rotação óptica de ESO-LV 5100550

    Science.gov (United States)

    Carvalho, D. B.; Soares, D. S. L.

    2003-08-01

    ESO-LV 5100550 é o membro mais fraco do par de galáxias austral SBG 357 (Soares et al. 1995). É classificada no catálogo RC3 como uma espiral ordinária de tipo inicial (early-type); porém, uma análise morfológica sugere que ela tenha uma grande barra. O objetivo do estudo é determinar sua cinemática de tal modo que possamos inferir mais a respeito de sua dinâmica, provavelmente perturbada, já que se espera que esteja sob forte influência da companheira ESO-LV 5100560. Apresentarei resultados parciais determinados a partir de espectros obtidos com o instrumento Double Spectrograph montado no telescópio Hale do Monte Palomar, EUA. As observações foram realizadas por D.S.L. Soares, P.M.V. Veiga e T.E. Nordgren, em 1998. Foram tomados espectros de fenda longa posicionada sobre a linha dos nodos do disco e ao longo da suposta barra. Os dados foram reduzidos com uso do pacote IRAF. Obtivemos o perfil de velocidades radiais na linha de visada ao longo das fendas e calculamos o desvio para o vermelho cosmológico do sistema, com base no espectro central. Determinamos as curvas de rotação deprojetadas, com base em cálculos para os valores teóricos esperados das componentes de velocidades puramente circulares em um disco inclinado. A inclinação do disco, dado fundamental nesta deprojeção, foi estimada através da média das elipticidades das isofotas mais externas.

  17. 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

  18. 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.

  19. 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...

  20. 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...

  1. The Expanding Fireball of Nova Delphini 2013

    CERN Document Server

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

    2015-01-01

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

  2. NOVA laser facility for inertial confinement fusion

    Energy Technology Data Exchange (ETDEWEB)

    Simmons, W.W.

    1983-11-30

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

  3. Enquête de satisfaction Novae

    CERN Multimedia

    2014-01-01

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

  4. Um novo paradigma para uma nova antropologia

    Directory of Open Access Journals (Sweden)

    Susin, Luiz Carlos

    2007-01-01

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

  5. Um algoritmo evolutivo híbrido para o problema de recobrimento de rotas com coletas de premios.

    OpenAIRE

    Silva, Matheus de Souza Alves; Mine, Marcio Tadayuki; Ochi, Luiz Satoru; Souza,Marcone Jamilson Freitas

    2010-01-01

    Este artigo propõe um algoritmo evolutivo híbrido para obter soluções aproximadas para o Problema de Recobrimento de Rotas com Coleta de Prêmios (PRRCP). O algoritmo proposto combina estratégias heurísticas baseadas nos procedimentos Busca Local Iterada, Busca em Vizinhança Variável, Reconexão por Caminhos e GENIUS. Resultados computacionais para um conjunto de instancias mostram a eficiência e a robustez da heurística proposta. _________________________________________________________________...

  6. 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

  7. 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...

  8. 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.

  9. 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.

  10. Unmanned aircraft system measurements of the atmospheric boundary layer over Terra Nova Bay, Antarctica

    Directory of Open Access Journals (Sweden)

    S. L. Knuth

    2013-02-01

    Full Text Available In September 2009, a series of long-range unmanned aircraft system (UAS flights collected basic atmospheric data over the Terra Nova Bay polynya in Antarctica. Air temperature, wind, pressure, relative humidity, radiation, skin temperature, GPS, and operational aircraft data were collected and quality controlled for scientific use. The data have been submitted to the United States Antarctic Program Data Coordination Center (USAP-DCC for free access (doi:10.1594/USAP/0739464.

  11. 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.

  12. 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

  13. 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

  14. 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

  15. 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...

  16. 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.

  17. 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.

  18. 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.

  19. 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.

  20. Estudo da configuração de rotas padrões de chegadas (STAR) RNAV através de simulação fast-time com a inclusão de rotas alternativas

    OpenAIRE

    Fernando Luiz Fantoni

    2015-01-01

    Rotas alternativas de chegada em área de controle terminal (TMA) demonstram ser uma opção para o gerenciamento de tráfego aéreo lidar com o crescente volume de aeronaves e consequentes desafios impostos na otimização da navegação horizontal e vertical destas. Porém, para que elas avancem da pesquisa para a implementação, é preciso compreender alguns aspectos tanto do lado da operação da aeronave quanto do controle de tráfego aéreo e ainda integrá-las à complexidade do ambiente operacional de...

  1. 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

  2. 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

  3. 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...

  4. 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.

  5. 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...

  6. 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.

  7. 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.

  8. 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.

  9. 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.

  10. /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.

  11. A Sutileza dos Quatérnions no Movimento de Rotação de Corpos Rígidos

    OpenAIRE

    Jambersi, Andreyson Bicudo [UNESP; Silva,Samuel da

    2016-01-01

    A parametrização da velocidade angular instantânea de um corpo rígido é usualmente descrita nos cursos de mecânica clássica com o auxílio dos ângulos de Euler. No entanto, para evitar problemas de singularidade na integração numérica das equações de movimento de rotação, outras formas de parametrização são mais interessantes. Dentre as diversas opções, os quatérnions são uma escolha bastante popular e com forte apelo prático na parametrização e integração das equações de Euler. Neste sentido,...

  12. Obtenção de materiais poliméricos mecanocrômicos por duas rotas

    OpenAIRE

    Westphal, Rafaela

    2012-01-01

    Dissertação (mestrado) - Universidade Federal de Santa Catarina, Centro Tecnológico, Programa de Pós-Graduação em Ciência e Engenharia de Materiais, Florianópolis, 2012 O presente trabalho tem como principal objetivo o desenvolvimento e a caracterização de materiais poliméricos com propriedades mecanocrômicas através de duas rotas: pela formação de cristais fotônicos e formação de excímeros. O domínio da técnica de fabricação de cristais fotônicos com propriedades elásticas ainda é recente...

  13. Radiation drive in laser heated hohlraums

    Energy Technology Data Exchange (ETDEWEB)

    Suter, L.J.; Kauffman, R.L.; Darrow, C.B. [and others

    1995-11-03

    Nearly 10 years of Nova experiments and analysis have lead to a relatively detailed quantitative and qualitative understanding of radiation drive in laser heated hohlraums. Our most successful quantitative modelling tool is 2D Lasnex numerical simulations. Analysis of the simulations provides us with insight into the details of the hohlraum drive. In particular we find hohlraum radiation conversion efficiency becomes quite high with longer pulses as the accumulated, high Z blow-off plasma begins to radiate. Extensive Nova experiments corroborate our quantitative and qualitative understanding.

  14. 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.

  15. 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.

  16. 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...

  17. 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

  18. 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....

  19. 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.

  20. 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.

  1. 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...

  2. 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.

  3. 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.

  4. 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...

  5. 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.

  6. 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...

  7. Non-Thermal Radio Emission from Colliding Flows in Classical Nova V1723 Aql

    CERN Document Server

    Weston, Jennifer H S; Metzger, Brian D; Zheng, Yong; Chomiuk, Laura; Krauss, Miriam I; Linford, Justin; Nelson, Thomas; Mioduszewski, Amy; Rupen, Michael P; Finzell, Tom; Mukai, Koji

    2015-01-01

    The importance of shocks in nova explosions has been highlighted by the recent discovery of \\gamma-ray producing novae by Fermi. We use over three years of multi-band radio observations of nova V1723 Aql with the Karl G. Jansky Very Large Array (VLA) to show that shocks between fast and slow flows within the ejecta led to the acceleration of particles and the production of synchrotron radiation. Approximately one month after the start of V1723 Aql's eruption in 2010 September, shocks in the ejecta produced an unexpected radio flare, ultimately resulting in a radio light curve with a multi-peaked structure. More than a year after the start of the eruption, the radio emission became consistent with emanating from an expanding thermal remnant with a mass of $2\\times10^{-4}$ M$_\\odot$ and a temperature of $10^4$ K. However, the brightness temperature of greater than $10^6$ K at low frequencies during the first two months was too high to be due to thermal emission from the small amount of X-ray producing shock-hea...

  8. Simulations and interpretation of the 6-cm MERLIN images of the classical nova V723 Cas

    CERN Document Server

    Heywood, I

    2007-01-01

    We compare the predictions of simple models for the radio emission from classical novae with the MERLIN radio observations of nova V723 Cas (Nova Cas 1995). Spherically symmetric and ellipsoidal radiative transfer models are implemented in order to generate synthetic emission maps. These are then convolved with an accurate representation of the uv coverage of MERLIN. The parameters and geometry of the shell model are based on those returned by fitting models to the observed light curve. This allows direct comparison of the model images with the nine 6-cm MERLIN images of V723 Cas. It is found that the seemingly complex structure (clumping, apparent rotation) evident in the observations can actually be reproduced with a simple spherical emission model. The simulations showthat a 24-h track greatly reduces the instrumental effects and the synthetic radio map is a closer representation of the true (model) sky brightness distribution. It is clear that interferometric arrays with sparse uv coverage (e.g. MERLIN, V...

  9. Produção de trigo e triticale em rotações de sequeiro Wheat and triticale in crop rotations

    Directory of Open Access Journals (Sweden)

    Carlos Castro

    2008-01-01

    Full Text Available Apresentam-se os resultados de um ensaio de rotações que decorreu durante dez anos em Vila Real (Trás-os-Montes. O ensaio incluiu a rotação tradicional das condições de sequeiro de Trás-os-Montes, cereal-alqueive (TA, e rotações alternativas susceptíveis de serem adoptadas nestas condições, cereal-leguminosa (TL, cereal-consociação forrageira (TC e cereal-prado de sequeiro (TP. Os cereais das rotações foram o trigo e, posteriormente, o triticale. Determinaram-se e analisaram-se as produções de grão e palha, os teores de nutrientes do grão e da palha e acompanharam-se os parâmetros do solo, pH, matéria orgânica e os teores de P2 O 5, K2 O e bases de troca. Destacam-se alguns resultados importantes, tais como: as produções de grão de cereal das rotações não mostrarem diferenças significativas entre si; a produção de palha da rotação TL ser superior às das restantes; o trigo cultivado após prado de sequeiro não dispensar a adubação azotada; as rotações conduzirem a modificações dos teores de matéria orgânica, cálcio de troca ou do valor do pH do solo, factores a que se deve atender, caso a rotação se prolongue por muitos anos.The results of a field trial of crop rotations conducted over a period of ten years in Vila Real (Northeast Portugal are presented. The rotations tested were cereal-cultivated fallow (TA, traditional in rain-fed conditions of the region, and alternative rotations that could be adopted in these conditions: cereal-grain legume crop (TL, cereal-forage mixture (TC and cereal-rain-fed pasture (TP. The cereals were wheat and, later, triticale. Grain, straw and aerial biomass yields were evaluated together with concentrations of nutrients. The soil parameters studied were pH, organic matter and P 2 O 5, K2O and exchange cations. Wheat straw yield of TL rotation was higher than that of the others. Wheat from TP rotation still requires nitrogen fertilization. The soils of the different

  10. Efetividade de um protocolo de reprocessamento na esterilização de canetas de alta-rotação em autoclave gravitacional

    OpenAIRE

    Alvarenga, Camila Fonseca; Reis, Cleomenes; Tipple,Anaclara Ferreira Veiga; Paiva,Enilza Maria Mendonça de; Sasamoto,Sandra Aragão de Almeida

    2011-01-01

    v.13,n.3,p.560--565,jul./set. 2011. Canetas odontológicas de alta-rotação são instrumentos de grande uso na prática clínica, com descontaminação polêmica, por apresentar complexo funcionamento. Estudo microbiológico, realizado no Serviço Odontológico da Universidade Federal de Goiás, teve como objetivo avaliar a efetividade do reprocessamento de canetas odontológicas de alta-rotação em autoclave gravitacional, seguindo um protocolo. Observados os aspectos éticos, os dados foram obtidos por...

  11. 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.

  12. 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...

  13. 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

  14. 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

  15. 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…

  16. 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:

  17. A Randomized Comparison between Video Demonstration and Verbal Instruction in Improving Rota Haler Technique in Children with Persistent Asthma: A Pilot Study.

    Science.gov (United States)

    Arumugom, Archana; Chandrasekaran, Venkatesh

    2017-06-01

    Inhalation therapy is the cornerstone in management of asthma. Failure to use the device properly is one of the factors incriminated in poor control of asthma. To compare the technique of rota haler use in children with persistent asthma immediately after receiving either verbal instruction or a video based demonstration and again at one month following intervention. A total of 28 children, older than six years attending the childhood asthma clinic of our hospital, who were prescribed rota halers for the first time and who were technique naïve were enrolled into the study, after obtaining informed consent from the parents after meeting inclusion and exclusion criteria. They were then randomly assigned to either verbal instructions (group of 14) or video demonstration group (group of 14), for teaching them the rota haler technique. Their technique was then assessed using a modified version of the inhaler device assessment tool immediately after education and one month after the intervention. The proportions of children with good technique in both groups at both time points were compared. There was no significant difference in the baseline variables like age, gender, location, socio-economic status and disease duration between both groups. The proportion of children achieving good technique was significantly more in the video group than the oral instruction group at immediate assessment and also at one month post intervention with an odds of 8 and 23.40 respectively (p=0.0262 and 0.0075 respectively). Video demonstration is effective in improving the technique of rota haler use at immediate assessment and at one month post intervention. Further studies are needed to validate this study and to assess factors that predict successful device use.

  18. 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.

  19. 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...

  20. 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 ...

  1. DETERMINAÇÃO DA ROTA ÓTIMA DE TRANSPORTE COM AUXÍLIO DE UM SISTEMA DE INFORMAÇÃO GEOGRÁFICA

    Directory of Open Access Journals (Sweden)

    Attilio Antonio Disperati

    2005-11-01

    Full Text Available O objetivo deste trabalho foi realizar uma análise comparativa entre os critérios de desempenho operacional do veículo e a menor distância na determinação da rota ótima no transporte florestal rodoviário, com auxílio de um sistema de informações geográficas. Inicialmente, foram realizadas a vetorização e a classificação de uma rede de estradas em uma empresa florestal. Em seguida, com auxílio do software Spring, versão 4.0, realizaram oito simulações de rota ótima de transporte, partindo-se de diferentes pontos locados ao acaso na área de estudo para um único destino. Os resultados indicaram que não houve diferença significativa na produtividade e no custo do transporte florestal entre os critérios analisados. Por outro lado, os resultados mostraram que o desempenho operacional foi o critério mais eficiente na determinação da rota ótima de transporte, comprovando a teoria de que nem sempre a menor distância é a mais econômica.

  2. FUSE Observations of the Bright, Eclipsing Nova-like Cataclysmic Variable, UX UMa (FUSE 2000)

    Science.gov (United States)

    Long, Knox; Froning, Cynthia

    2004-01-01

    This was a project to study the disk and wind of the eclipsing nova-like variable UX UMa, in order to better define the wind geometry of the system, including the nature of the transition region between the disk photosphere and the supersonic wind. We proposed to use phase resolved spectroscopy of the system, taking advantage of the fact that UX UMa is an eclipsing system, to isolate different regions of the wind and to use a Monte Carlo radiative transfer code to simulate the spectra through the eclipse.

  3. Nova symmetry: Experiments, modeling, and interpretation (HLP3 and HLP4)

    Energy Technology Data Exchange (ETDEWEB)

    Suter, L.J.; Hauer, A.A. [Los Alamos National Lab., NM (United States); Powers, L.V.

    1996-06-01

    Understanding and controlling capsule implosion symmetry is a key requirement for inertial confinement fusion (ICF). Symmetry was specifically called out in the Nova Technical Contract (NTC) as the HLP4 task. Later, elements of HLP3 were expanded to include symmetry work. For nearly a decade and a half it has been recognized that the fundamental asymmetry in a laser-heated hohlraum is a long-wavelength pole-waist radiation flux variation that varies like the P{sub 2} Legendre polynomial. It has also been recognized that one can control this asymmetry and achieve nearly symmetric implosions by appropriately pointing the laser beams.

  4. Unmanned aircraft system measurements of the atmospheric boundary layer over Terra Nova Bay, Antarctica

    Directory of Open Access Journals (Sweden)

    S. L. Knuth

    2012-11-01

    Full Text Available In September 2009, a series of long-range unmanned aircraft system (UAS flights collected basic atmospheric data over the Terra Nova Bay polynya in Antarctica. Air temperature, wind, pressure, relative humidity, radiation, skin temperature, GPS, and operational aircraft data were collected and quality controlled for scientific use. The data has been submitted to the United States Antarctic Program Data Coordination Center (USAP-DCC for free access (doi:10.1594/USAP/0739464.

  5. 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.

  6. 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...

  7. The theology of matrimonial law in speeches of Benedict XVI to the tribunal of the roman rota

    Directory of Open Access Journals (Sweden)

    Denilson Geraldo

    2015-07-01

    Full Text Available The speech of the Pope to the Roman Rota opens every year the work of this Apostolic Tribunal and is awaited with anticipation by those involved in the judicial action of the Church, becoming a reference for all ecclesiastical tribunals. Benedict XVI reflects on family in the legal perspective, but he bases his thinking in theology and philosophy with opening for anthropology. Divided into three groups, the article aims to expose the thought of Benedict XVI on the action of the tribunals and the direct contribution they have on the theology of marriage He considers the question of canonical hermeneutics in the same line of theological reflection on hermeneutics continuity that marked the Vatican II Council and recognizes the family as a divine and inscribed in human nature institution. The methodology used was direct contact with the texts published in the weekly newsletter of the Holy See and the completion of the work is that Benedict XVI elaborates a theology of matrimonial law open to dialogue, to the challenges of today's culture, rooted in human nature and in the sacrament.

  8. 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

  9. 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.

  10. 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.

  11. 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.

  12. 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.

  13. 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.

  14. 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.

  15. 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 ...

  16. 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.

  17. 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

  18. 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.

  19. 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....

  20. 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.

  1. 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.

  2. 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...

  3. Mass transfer variation in the outburst model of dwarf novae and soft X-ray transients

    CERN Document Server

    Viallet, M

    2008-01-01

    We discuss two mechanisms that could result in an enhancement of the mass transfer rate during outbursts of dwarf novae and soft X-ray transients: the hot outer disc rim itself could heat the L1 point and scattered radiation by optically thin outflowing matter could also heat L1 significantly. We determine quantitatively the increase of the mass transfer rate resulting from an extra heating. During outbursts, the disc edge heats up the upper layer of the secondary with a flux of the order of the intrinsic stellar flux. This probably has no large effect on the mass transfer rate. In soft X-ray transients, the environing medium of the disc (corona+wind) could back-scatter a certain fraction of the accretion luminosity toward L1. Since soft X-ray transients reach high luminosities, even a low efficiency of this effect could yield a significant heating of L1, whereas we show that in dwarf novae this effect is negligible. Initially the incoming radiation does not penetrate below the photosphere of the secondary. D...

  4. 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...

  5. 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...

  6. 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.

  7. 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...

  8. 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.

  9. 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.

  10. 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.

  11. 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).

  12. Efeito da mucuna e amendoim em rotação com algodoeiro A study on crop rotation for cotton using velvet bean and peanut

    Directory of Open Access Journals (Sweden)

    Carlos A. M. Ferraz

    1977-01-01

    Full Text Available O efeito da rotação de mucuna (Stizolobium atterrimum Piper & Tracy e amendoim (Arachis hypogaea L. e de duas variedades comerciais de algodoeiro, IAC RM3 e IAC 12-2 (Gossypium hirsutum L. foi estudado nos anos agrícolas de 1967/68 a 1972/73. Foram instalados dois ensaios, um em Presidente Bernardes, com fusariose, em solo podzolizado de Lins e Marília var. Lins naturalmente infectado por Fusarium oxysporumf. vasinfectum e o nematóide causador de galhas Meloidogyne incognita (Kofoid & White Chitwood, e outro em Presidente Venceslau, sem fusariose, em latossolo vermelho-escuro f. arenosa não infectado. A variedade comercial IAC RM3 é resistente e a IAC 12-2 é suscetível à fusariose. Para a análise estatística dos dados adotou-se o esquema de parcelas subdivididas, com seis repetições, tendo sido consideradas como parcelas as variedades de algodoeiro IAC RM3 e IAC 12-2, plantadas em 1968/69, 1970/71, 1971/72 e 1972/73, e como subparcelas as culturas em rotação, mucuna, amendoim e as variedades de algodoeiro IAC RM3 e IAC 12-2, plantadas nos anos-agrícolas de 1967/68 e 1969/70. Em solos com fusariose, em 1968/69, e em solos sem fusariose, no ano agrícola de 1970/71, destacou-se o efeito da rotação com mucuna, seguida da rotação com amendoim. Depois do plantio consecutivo de algodoeiro durante três anos (1970/71 a 1972/73, cessaram praticamente os efeitos da rotação para os dois casos. Houve aumento do teor de potássio após o primeiro ano de rotação, sendo maior para a mucuna.The effect of rotation of velvet bean (Stizolobium atterrimum Piper & Tracy, and peanut (Arachis hypogaea L. with two comercial varieties of cotton IAC RM3 and IAC 12-2 (Gossypium hirsutum L. was studied during 1967/68 to 1972/73. One experiment was conducted in a soil naturally infected by Fusarium oxysporum f. vasinfectum (Atk. Snyder & Hansen and by Meloidogyne incognita (Kofoid & White Chitwood, (President Bernardes, State of São Paulo, in

  13. 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...

  14. Efeitos da rotação de culturas na incidência de podridões radiciais e na produtividade da soja

    Directory of Open Access Journals (Sweden)

    Erlei Melo Reis

    2014-03-01

    Full Text Available Em experimentos conduzidos no campo, no sistema plantio direto, nas safras de verão de 2003/04, 2004/05 e 2005/06 foram avaliados os efeitos de culturas de inverno, da rotação e da monocultura sobre a emergência de plântulas, na incidência de podridões radiciais e no rendimento de grãos da soja. Demonstrou-se não haver efeitos das culturas de inverno sobre a emergência de plântulas da soja. Quanto à incidência de podridões radiciais em monocultura foi registrada uma intensidade de até 99,2%. O maior rendimento de grãos foi obtido na soja cultivada em rotação com uma safra com milho. Os fungos isolados do sistema radicial de plantas infectadas foram, Macrophomina phaseolina, Phomopsis sp., Fusarium spp. e Colletotrichum truncata. O solo da área experimental pode ser considerado supressivo aos fatores que reduzem a germinação, a emergência de plântulas e de morte de plântulas/plantas de soja. Quanto ao seu efeito em reduzir as podridões radiciais, ainda não se detectou efeito supressivo, porém a rotação da soja com o milho reduziu a incidência de podridões radiciais e aumentou o rendimento de grãos da soja.

  15. Estabelecimento de rotação econômica para uma floresta regulada Establishment of economic rotation for a regulated forest

    Directory of Open Access Journals (Sweden)

    Márcio Lopes da Silva

    2006-02-01

    Full Text Available O objetivo deste trabalho foi determinar as rotações econômicas para um povoamento florestal, considerando-se um único corte e infinitos cortes, e para uma floresta regulada, por meio de modelos matemáticos, bem como compará-las através da análise marginal das condições de otimalidade. Para validar o modelo e verificar a magnitude dos efeitos, foi utilizado um estudo de caso de um projeto florestal com valores reais de produção, custos, receitas e taxa de desconto. Os resultados indicaram que os modelos foram eficientes para determinar a rotação econômica e que a rotação do povoamento para um único corte e infinitos cortes e para a floresta regulada foi, respectivamente, de 6,5; 5,5; e 5 anos. O Valor Esperado do Solo (VES para a floresta regulada foi inferior ao VES do povoamento, em virtude de se impor ao manejo a condição de regulação.The objective of this work was to determine the economic rotations for a forest stand taking into considereation only one harvest, infinite harvests and a regulated forest using mathematical models, as well as comparing them through the marginal analysis of optimality conditions. To validate the model and to verify the magnitude of the effect a study case of a forest project, with real values of production, costs, revenues and discounting rate, was used. The results indicated that the models were efficient to determine the economic rotation and that the rotation of the stand for one cut, infinite cuts and for the regulated forest were respectively 6.5, 5.5 and 5 years. The Soil Expectation Value (SEV for the regulated forest was smaller than the SEV of the stand due toimposed regulations on the forest management.

  16. Avaliação do déficit de rotação medial e do encurtamento posterior do ombro em jogadores profissionais de basquetebol

    Directory of Open Access Journals (Sweden)

    Valquíria Nunes

    2012-06-01

    Full Text Available O arremesso destaca-se como um dos principais gestos que envolvem a articulação do ombro. Atletas que praticam arremessos acima da cabeça possuem maior propensão a desenvolver lesões no ombro e podem apresentar significativo aumento da rotação lateral (RL e diminuição da rotação medial (RM. O déficit de RM é chamado GIRD (glenohumeral internal rotation deficit. O objetivo do estudo foi verificar a existência de alterações na mobilidade da articulação glenoumeral em atletas profissionais de basquetebol, bem como verificar se existe correlação entre a ADM de RM e o encurtamento posterior do ombro. MÉTODO: Foram avaliados 19 jogadores profissionais de basquetebol. A mensuração da RM e RL do ombro foi realizada através dos métodos de goniometria e biofotogrametria, e também foi realizado o teste para encurtamento posterior do ombro. RESULTADOS: Não foram observadas diferenças significantes entre os gêneros e também entre as rotações (RL e RM quando comparados o ombro dominante e o não dominante, assim como, no teste de encurtamento posterior, não foram observadas diferenças estatisticamente significantes. Não houve correlações entre a diminuição de RM e o teste para encurtamento posterior do ombro. CONCLUSÃO: Alterações na mobilidade da articulação glenoumeral em atletas profissionais de basquetebol não foram encontradas nessa amostra, assim como não houve correlação entre a ADM de RM e o encurtamento posterior do ombro.

  17. 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.

  18. Rotas de preparação de intermediarios para a sintese de alcaloides indolicos e extração de produtos naturais relacionados

    OpenAIRE

    Antonio Carlos Siani

    1980-01-01

    Resumo: No presente trabalho são apresentadas rotas de preparação de moléculas intermediárias chaves (sintones) que posteriormente possam conduzir à alcalóides indólicos do tipo Vinca (vincamina, erbunamonina - hipotensores cerebrais) e Stricnos (estricnina). O projeto de pesquisa resume-se em duas etapas: a preparação de substratos imídicos (N-(o) toluilglutarimida, N-(o)toluilglutaconimida, N-(o) toluilmaleimida e derivados) e no comportamento desses substratos em meio básico. A ação da bas...

  19. Active head rotation in benign positional paroxysmal vertigo Da rotação cefálica ativa na vertigem posicional paroxística benigna

    Directory of Open Access Journals (Sweden)

    Fernando Freitas Ganança

    2009-08-01

    Full Text Available Benign Positional Paroxysmal Vertigo (BPPV is one of the most common vestibular diseases and the active head rotation test one of the most modern methods of vestibular function assessment. AIM: this study aims to verify if the active head rotation test may reveal signs of horizontal and/or vertical vestibulo-ocular reflex dysfunction in vertigo patients suspected for BPPV. STUDY DESIGN: retrospective series study. MATERIALS AND METHOD: Neurotological evaluation including computerized electronystagmography and active head rotation on the horizontal and vertical axes were conducted in 100 patients suspected for BPPV patients. Results: Isolated or associated abnormalities of the horizontal and/or vertical vestibulo-ocular reflex gain, phase and symmetry were indicative of vestibular involvement and found in 77.0% of the BPPV patients. CONCLUSION: the active head rotation test revealed horizontal and/or vertical vestibulo-ocular reflex dysfunctions in a relevant number of BPPV patients.A vertigem posicional paroxística benigna (VPPB corresponde a uma das vestibulopatias mais comuns e a rotação cefálica ativa um dos métodos mais modernos de avaliação da função vestibular. OBJETIVO: O objetivo desta pesquisa foi verificar se a prova de rotação cefálica ativa pode revelar sinais de disfunção do reflexo vestíbulo-ocular horizontal e/ou vertical em pacientes vertiginosos com hipótese diagnóstica de VPPB. DESENHO DO ESTUDO: Estudo de série retrospectivo. MATERIAL E MÉTODO: Uma avaliação otoneurológica incluindo a eletronistagmografia computadorizada e a prova de rotação cefálica ativa, no plano horizontal e vertical foi conduzida em 100 pacientes com hipótese diagnóstica de VPPB. Resultados: Alterações isoladas ou associadas de ganho, fase e assimetria do reflexo vestíbulo-ocular horizontal e/ou vertical, foram os achados indicativos de comprometimento vestibular em 77,0% dos casos de VPPB. CONCLUSÃO: A prova de rota

  20. Criação de rotas de entrega de produtos e recolha de paletes : aplicação à A Padaria Portuguesa

    OpenAIRE

    Pereira, Diogo Rafael Parreiras

    2016-01-01

    Mestrado em Decisão Económica e Empresarial Este estudo foi feito juntamente com um estágio na organização "A Padaria Portuguesa" e tem como principal objetivo a obtenção de rotas de distribuição de produtos e a recolha de paletes, bem como a aferição das atualmente utilizadas. Inicialmente, o estágio visou o conhecimento do funcionamento de uma organização, bem-sucedida, como "A Padaria Portuguesa", com especial foco no tipo de infraestrutura. Este período, utilizado para a recolha de ...

  1. 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....

  2. 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...

  3. 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.

  4. 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.

  5. 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.

  6. Magnetic Gradient Horizontal Operator (MHGO) useful for detecting objects buried at shallow depth: cultural heritage (Villa degli Antonini, Rota Rio)

    Science.gov (United States)

    Di Filippo, Michele; Di Nezza, Maria

    2016-04-01

    Several factors were taken into consideration in order to appropriately tailor the geophysical explorations at the cultural heritage. Given the fact that each site has been neglected for a long time and in recent times used as an illegal dumping area, we thoroughly evaluated for this investigation the advantages and limitations of each specific technique, and the general conditions and history of the site. We took into account the extension of the areas to be investigated and the need for rapid data acquisition and processing. Furthermore, the survey required instrumentation with sensitivity to small background contrasts and as little as possible affected by background noise sources. In order to ascertain the existence and location of underground buried walls, a magnetic gradiometer survey (MAG) was planned. The map of the magnetic anomalies is not computed to reduction at the pole (RTP), but with a magnetic horizontal gradient operator (MHGO). The magnetic horizontal gradient operator (MHGO) generates from a grid of vertical gradient a grid of steepest slopes (i.e. the magnitude of the gradient) at any point on the surface. The MHGO is reported as a number (rise over run) rather than degrees, and the direction is opposite to that of the slope. The MHGO is zero for a horizontal surface, and approaches infinity as the slope approaches the vertical. The gradient data are especially useful for detecting objects buried at shallow depth. The map reveals some details of the anomalies of the geomagnetic field. Magnetic anomalies due to walls are more evident than in the total intensity map, whereas anomalies due to concentrations of debris are very weak. In this work we describe the results of an investigation obtained with magnetometry investigation for two archaeological sites: "Villa degli Antonini" (Genzano, Rome) and Rota Ria (Mugnano in Teverina, Viterbo). Since the main goal of the investigation was to understand the nature of magnetic anomalies with cost

  7. Uso e rotação de opioides para dor crônica não oncológica

    Directory of Open Access Journals (Sweden)

    Durval Campos Kraychete

    2012-08-01

    Full Text Available JUSTIFICATIVA E OBJETIVOS: Para o tratamento da dor crônica existe a possibilidade de uso prolongado de opioides. Os opioides são eficazes para praticamente todas as síndromes dolorosas crônicas não oncológicas, porém podem causar dependência. O objetivo deste texto é fazer uma revisão sobre o uso e rotação de opioides para dor crônica não oncológica. CONTEÚDO: O uso de opioides potentes é controverso e não são recomendados como medicamentos de primeira linha devido à possibilidade de dependência. Foi descrita tolerância, vício, fatores de risco para vício, rotação ou troca, regras gerais para administração, tabelas de conversão e dicas para prescrição de opioides. CONCLUSÕES: Os opioides são fármacos com eficácia comprovada para dor crônica não oncológica, porém sua prescrição deve ser feita respeitando alguns critérios para reduzir a incidência de efeitos adversos e vício.

  8. 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.

  9. π0 mass reconstruction in NOvA Far Detector.

    Science.gov (United States)

    Edayath, Sijith

    2017-01-01

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

  10. Fermi Reveals New Light on Novae in Gamma rays

    CERN Document Server

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

    2016-01-01

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

  11. Fabrication and testing of gas-filled targets for large-scale plasma experiments on nova

    Energy Technology Data Exchange (ETDEWEB)

    Stone, G.F.; Rivers, C.J.; Spragge, M.R.; Wallace, R.J.

    1996-06-01

    The proposed next-generation ICF facility, the National Ignition Facility (NIF) is designed to produce energy gain from x-ray heated {open_quotes}indirect-drive{close_quotes} fuel capsules. For indirect-drive targets, laser light heats the inside of the Au hohlraum wall and produces x rays which in turn heat and implode the capsule to produce fusion conditions in the fuel. Unlike Nova targets, in NIF-scale targets laser light will propagate through several millimeters of gas, producing a plasma, before impinging upon the Au hohlraum wall. The purpose of the gas-produced plasma is to provide sufficient pressure to keep the radiating Au surface from expanding excessively into the hohlraum cavity. Excessive expansion of the Au wall interacts with the laser pulse and degrades the drive symmetry of the capsule implosion. The authors have begun an experimental campaign on the Nova laser to study the effect of hohlraum gas on both laser-plasma interaction and implosion symmetry. In their current NIF target design, the calculated plasma electron temperature is T{sub e} {approx} 3 keV and the electron density is N{sub e} {approx} 10{sup 21}cm{sup {minus}3}.

  12. HST Images Flash Ionization of Old Ejecta by the 2011 Eruption of Recurrent Nova T Pyxidis

    CERN Document Server

    Shara, Michael M; Schaefer, Bradley E; Bond, Howard E; Godon, Patrick; Mac Low, Mordecai-Mark; Pagnotta, Ashley; Prialnik, Dina; Sion, Edward M; Toraskar, Jayashree; Williams, Robert E

    2015-01-01

    T Pyxidis is the only recurrent nova surrounded by knots of material ejected in previous outbursts. Following the eruption that began on 2011 April 14.29, we obtained seven epochs (from 4 to 383 days after eruption) of Hubble Space Telescope narrowband Ha images of T Pyx . The flash of radiation from the nova event had no effect on the ejecta until at least 55 days after the eruption began. Photoionization of hydrogen located north and south of the central star was seen 132 days after the beginning of the eruption. That hydrogen recombined in the following 51 days, allowing us to determine a hydrogen atom density of at least 7e5 cm^-3 - at least an order of magnitude denser than the previously detected, unresolved [NII] knots surrounding T Pyx. Material to the northwest and southeast was photoionized between 132 and 183 days after the eruption began. 99 days later that hydrogen had recombined. Both then (282 days after outburst) and 101 days later, we detected almost no trace of hydrogen emission around T Pyx...

  13. The slow decline of the Galactic recurrent novae T Pyxidis, IM Normae, and CI Aquilae

    CERN Document Server

    Caleo, Andrea

    2015-01-01

    A distinguishing trait of the three known Galactic recurrent novae with the shortest orbital periods, T Pyx, IM Nor, and CI Aql, is that their optical decline time-scales are significantly longer than those of the other recurrent systems. On the other hand, some estimates of the mass of the ejecta, the velocity of the ejecta, and the duration of the soft X-rays emission of these systems are of the order of those of the other recurrent systems and the fast classical novae. We put forth a tentative explanation of this phenomenon. We propose that in these systems part of the material transferred from the companion during the first few days of the eruption remains within the Roche lobe of the white dwarf, preventing the radiation from ionizing the ejecta of the system and increasing the optical decline time-scale. We explain why this phenomenon is more likely in systems with a high mass transfer rate and a short orbital period. Finally, we present a schematic model that shows that the material transferred from th...

  14. Cuento: Agua rota

    Directory of Open Access Journals (Sweden)

    José Puben

    1966-04-01

    Full Text Available Ya avanzada la noche la lluvia empezó a caer, clara y sonora, en el empedrado del patio y sobre los amplios techos de la vieja casa. El ruido del aguacero lo despertó de un profundo sueño. La sensación de que la cañada aumentaba, a cada momento, venía del atronador y permanente cauce de las aguas vecinas.

  15. 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...

  16. 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...

  17. 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-...

  18. 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.

  19. 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

  20. 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.

  1. 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.

  2. 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

  3. 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.

  4. 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 .

  5. 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.

  6. 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.

  7. 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.

  8. Viscosidade como fator frenador de rotações Viscoelastic substances as a breaking factor of ocular rotations

    Directory of Open Access Journals (Sweden)

    André Augusto Homsi Jorge

    2003-08-01

    Full Text Available OBJETIVO: Determinar se forças de atrito viscoso podem, sob o ponto de vista quantitativo, agir como possíveis promotoras de estabilização ocular com manutenção dos movimentos de rotação, dando noção dos valores necessários para a aplicabilidade no sistema ocular. MÉTODOS: Um modelo mecânico foi elaborado para a medida de forças necessárias para vencer o atrito de uma esfera de alumínio parcialmente mergulhada em um líquido viscoso. Foram testadas soluções de metilcelulose de 1% a 6% (com variação de 0,5% e dois produtos viscoelásticos (Viscoat® e Provisc®. Outra variável foi a área de contato entre a esfera e o líquido viscoso. RESULTADOS: A força encontrada, após correções e descontos apropriados, foi significativa (acima de 5 gf apenas nas soluções de metilcelulose 5,5% e 6% e somente na maior área de contato testada. CONCLUSÃO: Os líquidos viscosos testados aparentemente não são capazes de obter força de atrito suficiente para a estabilização ocular, com exceção das soluções de metilcelulose 5,5% e 6% mas somente na maior área de contato testada (que correspondeu a 26,2% da área total da esfera.PURPOSE: The aim of this study was to find out if the viscous friction forces could, from the quantitative point of view, act as possible promoters of ocular stabilization keeping the rotational movements and give an idea of the necessary amount for the applicability to the ocular system. METHODS: A mechanic model was made to measure the necessary forces to overcome the friction of the aluminium sphere partially kept in a viscous liquid. Methylcellulose solutions at 1% to 6% (with a variation of 0.5% and viscoelastic products (Viscoat® and Provisc® were tested. Another variable was the area of contact between the sphere and the viscous liquid. RESULTS: The force that was found, after appropriate corrections and discounts, was meaningful (over 5 gf only in the of methylcellulose solutions at 5.5% and 6

  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. "Anti-glitches" in the Quark-Nova model for AXPs

    CERN Document Server

    Ouyed, Rachid; Koning, Nico

    2013-01-01

    In the Quark-Nova model, AXPs are quark stars surrounded by a degenerate iron-rich Keplerian ring (a few stellar radii away). AXP bursts are caused by accretion of chunks from the inner edge of the ring following magnetic field penetration. For bright bursts, the inner disk is prone to radiation induced warping which can tilt it into counter-rotation (i.e. retrograde). For AXP 1E2259+586, the 2002 burst satisfies the condition for the formation of a retrograde inner ring. We hypothesize the 2002 burst reversed the inner ring setting the scene for the 2012 outburst and "anti-glitch" when the retrograde inner ring was suddenly accreted leading to the basic observed properties of the 2012 event.

  14. Efeito da rotação da cabeça na pressão intraocular em decúbito ventral: estudo randomizado

    Directory of Open Access Journals (Sweden)

    M. Nuri Deniz

    2013-04-01

    Full Text Available JUSTIFICATIVA E OBJETIVOS: A elevação da pressão intraocular (PIO, que diminui a pressão de perfusão do nervo óptico, é aumentada pelo posicionamento em decúbito ventral. O objetivo de nosso estudo foi comparar o efeito da rotação lateral da cabeça a 45º em decúbito ventral no aumento da PIO de olhos posicionados para cima e olhos posicionados para baixo em pacientes submetidos à nefrolitotomia percutânea (NLPC. MÉTODOS: Quarenta e cinco pacientes foram randomicamente alocados em dois grupos. A PIO dos pacientes foi registrada bilateralmente em posição supina antes do início da operação. Os pacientes foram posicionados em decúbito ventral. A cabeça foi posicionada sobre um apoio sem compressão externa direta em ambos os olhos. Os pacientes do Grupo I foram estritamente mantidos em pronação neutra, enquanto os pacientes do Grupo II foram posicionados em pronação com rotação da cabeça a 45º para o lado direito. No fim da operação, os pacientes foram reposicionados em decúbito dorsal e a PIO foi imediatamente medida. RESULTADOS: Não houve diferença entre os dados demográficos, na duração da cirurgia, perda de sangue e reposição de líquido dos pacientes. Os valores pós-cirúrgicos da PIO em decúbito ventral aumentaram significativamente em comparação com os valores pré-operatórios em ambos os grupos (p < 0,05. Após a cirurgia em decúbito ventral, os valores da PIO nos olhos posicionados para cima no Grupo II foram significativamente menores do que no Grupo I e nos olhos posicionados para baixo no Grupo II (p < 0,05. CONCLUSÃO: A posição em decúbito ventral aumenta a PIO. Nos pacientes posicionados em decúbito ventral com rotação lateral da cabeça a 45º, a PIO nos olhos posicionados para cima foi significativamente menor.

  15. 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

  16. 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.

  17. 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.

  18. 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.

  19. 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

  20. 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.

  1. 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.

  2. 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...

  3. 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...

  4. 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

  5. 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

  6. 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)

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

    NARCIS (Netherlands)

    Eisner, C.

    1957-01-01

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

  8. 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.

  9. 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.

  10. 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…

  11. 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.

  12. 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.

  13. Auto-rotação cefálica ativa em pacientes com tontura/ vertigem Active cephalic auto-rotation in patients with dizziness/ vertigo

    Directory of Open Access Journals (Sweden)

    Aída R.M. de Assunção

    Full Text Available Introdução: A auto-rotação cefálica ativa é um teste rápido, de simples realização, não invasivo, que não causa desconforto ao paciente, pode ser realizado com facilidade em crianças e avalia o reflexo vestíbulo-ocular nas freqüências fisiológicas de movimentação da cabeça, utilizadas na vida cotidiana (de 1 a 4 Hz. Forma de estudo: clínico retrospectivo não randomizado. Objetivo: Avaliar pacientes com queixas de tontura/vertigem através da auto-rotação cefálica ativa comparando os sintomas com as alterações encontradas. Material e método: Um grupo de 1281 pacientes com queixa de tontura/vertigem foi submetido ao teste de auto-rotação cefálica ativa horizontal com alvo fixo, como uma etapa da avaliação otoneurológica. Resultados: As idades variaram de três a 93 anos com média de 49,6 anos, sendo 946 (73,8% do sexo feminino e 335 (26,2% do sexo masculino. A queixa de vertigem foi relatada por 896 (69,9% dos pacientes e a tontura por 385 (30,1%. A faixa de freqüência de resposta à prova de auto-rotação cefálica variou de 1,5 a 7,5Hz com média de 3,5Hz. A prova de auto-rotação cefálica ativa foi normal em 937 (73,1% e alterada em 344 (26,9% dos pacientes. As alterações mais freqüentes foram as relacionadas ao ganho (aumento, redução isoladas ou associadas a alterações de fase e simetria, em 241 (19% pacientes. O aumento do ganho isolado foi verificado em 92 pacientes (7,2%. Conclusão: Não houve relação entre as alterações na prova de auto-rotação cefálica ativa horizontal e as queixas de tontura e vertigem.Introduction: Active cephalic auto-rotation is a rapid, easy, painless and comfort test, that can be done in children and evaluate the vestibulo-ocular reflex in the physiologic frequencies of head, used in the every day life (from one to four hertz. Study design: clinical retrospective not randomized. Aim: Evaluate patients with complaints of dizziness/vertigo through the active

  14. 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...

  15. 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...

  16. 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)

  17. 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)

  18. 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...

  19. 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 ...

  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. 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.

  5. 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.

  6. 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.

  7. 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.

  8. 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.

  9. Erupting Dwarf Novae in the Large Magellanic Cloud

    CERN Document Server

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

    2003-01-01

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

  10. High Energy Neutrino Physics with NOvA

    Energy Technology Data Exchange (ETDEWEB)

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

    2016-09-09

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

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

    OpenAIRE

    Maraldi, Elisa

    2015-01-01

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

  12. Three new optical nova candidates in M 31

    Science.gov (United States)

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

    2011-06-01

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

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

    Science.gov (United States)

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

    2017-03-01

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

  14. 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

  15. 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, ...

  16. 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...

  17. 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 ...

  18. 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...

  19. 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.

  20. Efeito da rotação do quadril na síndrome da dor femoropatelar Effect of hip rotation on patellofemoral pain syndrome

    Directory of Open Access Journals (Sweden)

    K Gramani-Say

    2006-01-01

    Full Text Available Objetivo: A proposta desse trabalho foi investigar o efeito da rotação do quadril na atividade elétrica dos músculos Vasto Medial Oblíquo (VMO, Vasto Lateral Oblíquo (VLO e Vasto Lateral Longo (VLL no agachamento a 45º de flexão do joelho associado à posição neutra, rotação lateral a 45º e rotação medial a 15 e 30º de quadril. Materiais e Método: Foram avaliadas 27 mulheres, sendo 15 mulheres normais do grupo Controle (21,1±2,1 anos e 12 portadoras de Síndrome da Dor Femoropatelar (SDFP (21,0±2,3 anos. A atividade elétrica do músculo quadríceps foi captada por eletrodos ativos diferenciais simples de superfície, eletromiógrafo de 8 canais e programa Aqdados 7.2.6. Os dados foram normalizados pela porcentagem da média do agachamento a 75º com o quadril em posição neutra RMS (µV. A análise estatística utilizada foi a ANOVA two way com medidas repetidas e Turkey post hoc (pObjective: The purpose of this study was to evaluate the effect of hip rotation on the electrical activity of the Vastus Medialis Obliquus (VMO, Vastus Lateralis Obliquus (VLO and Vastus Lateralis Longus (VLL muscles when squatting with 45º knee flexion, in association with the neutral position, 45º lateral rotation and 15 and 30º medial hip rotation. Method: 27 women were evaluated: 15 healthy women as a control group (21.1 ± 2.1 years and 12 subjects with patellofemoral pain syndrome (PFPS (21.0 ± 2.3 years. The electrical activity of the quadriceps muscle was detected using simple active differential surface electrodes, an eight-channel electromyography system and the Aqdados 7.2.6 software. The data were normalized by the mean squatting percentage at 75º with the hip in the neutral position RMS (µV. Two-way ANOVA with repeated measurements followed by the Tukey post hoc test (p<0.05 was used for statistical analysis. Results: The results revealed interaction between groups and muscles (p=0.00, independent of hip position (p=0.39, and

  1. Caminhoneiros de rota curta e sua vulnerabilidade ao HIV, Santos, SP Vulnerability to HIV and AIDS of short distance truck drivers stationed, Brazil

    Directory of Open Access Journals (Sweden)

    Luciana Villarinho

    2002-08-01

    Full Text Available OBJETIVO: Descrever a vulnerabilidade, de caminhoneiros de rota curta, à transmissão sexual do HIV e da Aids. MÉTODOS: Foram entrevistados 279 caminhoneiros com vínculo de trabalho na cidade de Santos, SP, em locais de concentração na área portuária e suas proximidades, sindicatos e associações, recrutados pela amostragem do tipo "bola-de-neve". Foram realizadas entrevistas utilizando perguntas abertas e fechadas sobre questões sociodemográficas, práticas sexuais, uso de drogas, conhecimento sobre o HIV e a Aids, contato prévio com programas de prevenção à Aids em Santos, percepção de sua vulnerabilidade ao HIV e à Aids. Foi realizada análise descritiva da amostra, e apresentados relatos para ilustrar algumas situações de vulnerabilidade. RESULTADOS: Do total de 279 caminhoneiros entrevistados, 93% declararam ter parceira fixa, 40% referiram manter relações sexuais com parceiras casuais, e 19% referiram manter relações sexuais com parceiras freqüentes. A principal situação de vulnerabilidade ao HIV ocorre devido ao uso inconsistente do preservativo, interligado ao vínculo estabelecido com cada parceira. O tempo fora de casa parece não ser o principal fator para situações de vulnerabilidade, conforme demonstram estudos com caminhoneiros de rota longa. CONCLUSÕES: A cultura "machista" e os papéis tradicionais masculinos são emblemáticos entre os caminhoneiros de rota curta. Certamente é necessário investir mais na prevenção nessa categoria profissional. A prevenção em locais de trabalho parece promissora, pois permite entender melhor seu universo, propiciando intervenções educativas adequadas a essa categoria profissional.OBJECTIVE: To describe the vulnerability to sexually transmitted HIV/AIDS of short distance truck drivers. METHODS: Using a snowball sampling procedure, 279 truck drivers working in the port area and vicinities, unions and workers' associations of Santos, Brazil, were selected and

  2. Avaliação da amplitude de rotação interna da anca : comparação entre cadeias cinéticas aberta e fechada

    OpenAIRE

    Martins, João Pedro da Silva

    2013-01-01

    Mestrado em Exercício e Saúde A amplitude de rotação interna da anca tem sido avaliada no âmbito desportivo, sendo uma variável com relevância para a incidência de lesões. Essa avaliação é tipicamente efetuada em cadeia cinética aberta, ao contrário da maioria das ações desportivas em que esse movimento é executado em cadeia cinética fechada. O objetivo desta investigação foi avaliar e comparar a amplitude máxima de rotação interna da anca, em ambos os membros inferiores, em cadeia cinétic...

  3. Uma abordagem para a solução de problemas de rotações de tripulações para empresas aéreas utilizando busca tabu e janelas de tempo

    OpenAIRE

    Martins, Francisco José

    2007-01-01

    As escalas de tripulações em companhias aéreas é um fator importante na logística de operações dessas empresas e um problema interessante para a aplicação de Pesquisa operacional. Os custos com tripulantes no transporte aéreo são extremamente altos, superiores a 20% dos custos de operações das empresas. Diante desse contexto, este trabalho vem abordar o problema de rotações de tripulações em empresas aéreas. Uma rotação de tripulação – crew pairings – é uma seqüência de etapas ou segmentos de...

  4. 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.

  5. 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.

  6. Movimentos oculares e padrões de busca visual em tarefas de rotação mental Eye movements and scan patterns in mental rotation tasks

    Directory of Open Access Journals (Sweden)

    Priscila Covre

    2005-06-01

    Full Text Available O objetivo deste estudo é identificar as estratégias utilizadas nas tarefas de rotação mental pela análise dos traçados dos movimentos oculares. Foi analisado o desempenho de 40 participantes na comparação de pares de objetos tridimensionais rotacionados no eixo y, com diferenças de angulação de 0o a 180o. Foi utilizado um sistema computacional de rastreamento dos movimentos oculares (eyetracking durante a visualização de figuras. Os resultados mostram que tempo de julgamento, duração média das fixações do olho, número de fixações nos objetos e número de alternâncias entre os dois objetos aumentam em função da diferença de angulação. Análise dos traçados oculares, com base na inspeção visual, indica o uso de dois tipos de estratégias: rotação mental em torno dos eixos padrões e comparação independente da orientação. O uso dessas estratégias é discutido com relação ao desempenho dos participantes e à memória de trabalho.The purpose of this paper is to identify the strategies used on mental rotation tasks by analyzing ocular movements. The performance of 40 participants on comparison of pairs of three-dimensional objects, rotated on the y-axis, from 0o to 180o was analyzed. An eye-tracking computerized system was used to track eye movements during scene visualization. Results showed that judgment time, fixation duration, number of fixations and number of switches between the objects increased with rotation angle. Analysis by visual inspection indicates the use of two kinds of strategies: Mental rotation around the standard axis and comparison of orientation-free descriptions. The use of the strategies is discussed with regard to performance and working memory.

  7. 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.

  8. 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).

  9. 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.

  10. Dziesmas ar kustību un rotaļu elementiem vārdu krājuma apguvei angļu valodas nodarbībās pirmsskolā

    OpenAIRE

    Valdesa, Laura

    2015-01-01

    Tiek plaši uzskatīts, ka mūsdienās rotaļai un spēlei ir nozīmīga loma mācību procesā pirmskolā. Uzdevumi, kuri ir vispiemērotākie angļu valodas apmācībai pirmskolas vecumā ir tie, kas ietver dziesmas ar kustību un rotaļu elementiem, dzejoļus, stāstus, spēles un daudzas citas aktivitātes. Diplomdarba autore uzskata, ka viens no labākiem mācību un vārdu krājuma apguves veidiemdiem ir dziesmas ar kustību un rotaļu elementiem. Diplomdarbs tika izstrādāts, lai izpētīt priekšrocības izmantojot dzie...

  11. "4-5 gadus vecu bērnu matemātisko priekšstatu veidošanās latviešu rotaļdejā"

    OpenAIRE

    Matuseviča, Karīna

    2016-01-01

    4–5 gadus vecu bērnu matemātisko priekšstatu veidošanās latviešu rotaļdejā Autore–Karīna Matuseviča Zinātniskā vadītāja-profesore,Dr.paed.Rudīte Andersone Darba apjoms-52lpp., 1tabula, 5attēli, 4pielikumi, izmantoti 25literatūras avoti. Pētījuma mērķis–izpētīt 4–5gadus vecu bērnu matemātisko priekšstatu veidošanos latviešu rotaļdejā Pirmajā nodaļā analizēta matemātisko priekšstatu veidošanās pirmsskolā. Otrajā nodaļā veikta latviešu rotaļdeju teorētiskā analīze. Trešajā nodaļā aprakstīts 4 – ...

  12. 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...

  13. 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.

  14. 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.

  15. Chandra Discovers Eruption and Pulsation in Nova Outburst

    Science.gov (United States)

    2001-09-01

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

  16. Principais rotas de síntese de resinas complexantes de mercúrio Chelating resins for recovery of mercury: the main routes of synthesis

    Directory of Open Access Journals (Sweden)

    Luciana da Cunha

    2007-06-01

    Full Text Available A recuperação de espécies contendo mercúrio utilizando resinas complexantes obtidas a partir da modificação de suportes poliméricos vem atraindo cada vez mais a atenção dos pesquisadores. São muitas as combinações de suportes e grupos complexantes para a síntese desses materiais. Assim, este trabalho apresenta uma revisão sobre os principais grupos funcionais avaliados, bem como as rotas de síntese adotadas para a imobilização desses grupos nos suportes. É abordada também a problemática da síntese de uma resina eficiente, produzida a partir de um processo limpo e acessível às indústrias que utilizam mercúrio em seus processos.The recovery of mercury and its compounds by using chelating resins produced by modification of polymer supports has been studied by many researchers. There are many combinations of supports and functional groups for producing chelating resins that are appropriate for mercury complexation. This paper presents an overview of the main functional groups applied for mercury complexation and the routes used for immobilization of these groups in polymer supports. Also discussed are the problems involved in the synthesis of an efficient chelating resin, produced through a non-polluting route, which are appropriate for companies employing mercury in their processes.

  17. Bioetanol nos Estados Unidos: análise e perspectivas da produção e pesquisa focando as rotas bioquímicas

    Directory of Open Access Journals (Sweden)

    Rodolfo Freire Maiche

    2010-10-01

    Full Text Available O bioetanol, etanol lignocelulósico ou etanol de segunda geração é obtido a partir da sacarificação de celulose, hemicelulose e pectina presentes na parede celular de biomassas. O bioetanol está sendo amplamente estimulado nos Estados Unidos por ser um substituto direto da gasolina, não competir com culturas agrícolas destinadas à alimentação e por causar menos impacto ambiental. A celulose é o polissacarídeo mais abundante na terra, entretanto esta molécula é muito bem protegida na parede celular de plantas, e hidrolisá-la eficientemente a açúcares fermentáveis para produzir bioetanol a preços competitivos se tornou um dos maiores desafios da biotecnologia moderna. Esta revisão objetiva avaliar a produção e pesquisa de bioetanol nos Estados Unidos focando as rotas bioquímicas.

  18. Demanda energética de uma semeadora-adubadora em diferentes velocidades de deslocamento e rotações do motor Energy needs of a planter at different travel and engine speeds

    Directory of Open Access Journals (Sweden)

    João Cleber Modernel da Silveira

    2013-03-01

    Full Text Available A velocidade de operação do trator influencia diversos aspectos, entre eles o consumo de combustível, a capacidade operacional e a qualidade de semeadura. Este trabalho teve como objetivo avaliar a demanda energética de um conjunto trator-semeadora-adubadora em sistema plantio direto, em função das velocidades de deslocamento e rotações no eixo do motor, na semeadura da cultura do milho. Os 12 tratamentos foram constituídos de quatro velocidades de deslocamento, obtidas em função dos escalonamentos de marchas e de três rotações do motor do trator. Durante a semeadura, monitoraram-se a velocidade de operação, a rotação do motor, a força de tração e o consumo horário de combustível. Os resultados mostraram que o requerimento de potência na barra de tração, média, por linha de semeadura, por profundidade do sulco e por área mobilizada aumentou com o aumento da velocidade de operação do conjunto mecanizado. O consumo horário de combustível foi elevado com o aumento da velocidade de operação e da rotação do motor, sendo menor na rotação do motor de 1.500 rpm.The operating speed of the tractor influences various aspects, including fuel consumption, operational capacity and sowing quality. This study aimed to assess the energy needs of a tractor-planter when sowing maize in a no-tillage system, according to its travel speed and the rotation speed of the motor shaft. The 12 treatments consisted of four travel speeds, obtained by staggering the gears, and three tractor-engine rotation speeds. During sowing, the speed of operation, engine speed, the traction force and hourly consumption of fuel were monitored. The results showed that the average power requirement on the drawbar per seeding row, groove depth, and worked area, increased with an increase in the operating speeds of the mechanism. Hourly fuel consumption went up with the increase in operating and engine-rotation speeds, being lowest at a speed of 1,500 rpm.

  19. 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.

  20. 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.

  1. A rotação de cultura reduz a matocompetição e aumenta o teor de clorofila e a produtividade do arroz Crop rotation reduces weed competition and increases chlorophyll concentration and yield of rice

    Directory of Open Access Journals (Sweden)

    Ricardo Antonio Marenco

    1999-10-01

    Full Text Available A rotação de culturas é uma prática importante em sistemas agrícolas sustentáveis pelos efeitos benéficos tanto na fertilidade do solo como na redução da matocompetição, entre outros. Este trabalho foi conduzido no campo experimental da UEMA, em São Luís, MA. Avaliou-se o efeito da rotação de culturas na incidência de plantas invasoras, nos teores de clorofila e na produtividade do arroz (Oryza sativa L. cv. Guarani. Cultivou-se o arroz com e sem adubação nitrogenada, bem como em rotação com caupi (Vigna unguiculata (L. Walp., crotalária (Crotalaria paulina Schrank e mucuna (Mucuna aterrima Piper & Tracy. No primeiro ciclo a cobertura morta das leguminosas, deixada sobre o solo para a safra seguinte, foi máxima na crotalária, intermediária na mucuna e mínima no caupi. No segundo ciclo, cultivado em plantio direto sem uso de herbicidas, a rotação com mucuna e crotalária reduziu a biomassa, a cobertura e a densidade das invasoras. O teor de clorofila foi maior na rotação com crotalária do que na testemunha. A produtividade do arroz foi maior na rotação com crotalária e mucuna do que no arroz em cultivo sucessivo com ou sem N. Concluiu-se que a rotação do arroz com leguminosas aumenta a produtividade do arroz e reduz a matocompetição.Crop rotation is an essential practice in sustainable agricultural systems, because its effects on soil fertility and other benefits including reduction on weed competition. A field experiment was carried out at the UEMA experimental station, São Luís, Maranhão State, Brazil, to evaluate the effect of crop rotation on weed population, leaf chlorophyll concentration and yield of rice (Oryza sativa L. cv. Guarani. The rice was cultivated with and without N application, and in rotation with cowpea (Vigna unguiculata (L. Walp., hyacinthbean (Crotalaria paulina Schrank and velvetbean (Mucuna aterrima Piper & Tracy. First crop legume residues were highest in hyacinthbean, less in

  2. 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.

  3. 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.

  4. 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...

  5. 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.

  6. 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...

  7. 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...

  8. 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...

  9. 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.

  10. 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...

  11. 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...

  12. 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.

  13. 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.

  14. 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.

  15. 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...

  16. 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.

  17. 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…

  18. 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,...

  19. The physics of radiation driven ICF hohlraums

    Energy Technology Data Exchange (ETDEWEB)

    Rosen, M.D.

    1995-08-07

    On the Nova Laser at LLNL, we have recently demonstrated many of the key elements required for assuring that the next proposed laser, the National Ignition Facility (NIF) will drive an Inertial Confinement Fusion (ICF) target to ignition. The target uses the recently declassified indirect drive (sometimes referred to as {open_quotes}radiation drive{close_quotes}) approach which converts laser light to x-rays inside a gold cylinder, which then acts as an x-ray {open_quotes}oven{close_quotes} (called a hohlraum) to drive the fusion capsule in its center. On Nova we`ve demonstrated good understanding of the temperatures reached in hohlraums and of the ways to control the uniformity with which the x-rays drive the spherical fusion capsules. In this lecture we briefly review the fundamentals of ICF, and describe the capsule implosion symmetry advantages of the hohlraum approach. We then concentrate on a quantitative understanding of the scaling of radiation drive with hohlraum size and wall material, and with laser pulse length and power. We demonstrate that coupling efficiency of x-ray drive to the capsule increases as we proceed from Nova to the NIF and eventually to a reactor, thus increasing the gain of the system.

  20. 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.

  1. 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...

  2. 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...

  3. 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...

  4. 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 ...

  5. 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...

  6. 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.

  7. 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.

  8. 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...

  9. 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 ...

  10. 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.

  11. Uma nova cidade para as águas urbanas

    Directory of Open Access Journals (Sweden)

    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.

  12. 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.

  13. Radiation Protection

    Science.gov (United States)

    ... EPA United States Environmental Protection Agency Search Search Radiation Protection Share Facebook Twitter Google+ Pinterest Contact Us Radiation Protection Document Library View and download EPA radiation ...

  14. Spectral eclipse mapping of the accretion disk in the nova-like variable UX Ursae Majoris

    Science.gov (United States)

    Rutten, R. G. M.; Dhillon, V. S.; Horne, K.; Kuulkers, E.

    1994-01-01

    We analyze narrow-band eclipse light curves of the nova-like cataclysmic variable UX UMa, obtained from low-resolution spectra spanning lambda lambda 3600-9800 A . The light curves for narrow bands in the continuum as well as those for individual spectral lines are treated independently, and are used to construct images of the accretion disk's brightness distribution using the maximum-entropy eclipse-mapping technique. Particular attention is paid to the propagation of statistical uncertainties in the data and to how the analysis may introduce systematic errors in the final result. From the many narrrow band images we have reconstructed the spectra from isolated parts of the accretion disk. These spectra reveal that the inner disk radiates a continuum spectrum which peaks in the near UV and has the hydrogen Balmer lines in absorption (with the exception of H-alpha), whereas the outer disk is much fainter, has a much redder spectrum, and has Balmer emission lines. Our analysis reveals the presence of an uneclipsed component of the total light, whose spectrum is very red and has Balmer lines in emission. This unexpected feature of the eclipse mapping technique offers a new tool for an independent assessment of the secondary star's spectrum in eclipsing cataclysmic variables.

  15. Rise and fall of the dust shell of the classical nova V339 Delphini

    Science.gov (United States)

    Evans, A.; Banerjee, D. P. K.; Gehrz, R. D.; Joshi, V.; Ashok, N. M.; Ribeiro, V. A. R. M.; Darnley, M. J.; Woodward, C. E.; Sand, D.; Marion, G. H.; Diamond, T. R.; Eyres, S. P. S.; Wagner, R. M.; Helton, L. A.; Starrfield, S.; Shenoy, D. P.; Krautter, J.; Vacca, W. D.; Rushton, M. T.

    2017-01-01

    We present infrared spectroscopy of the classical nova V339 Del, obtained over a ˜2 year period. The infrared emission lines were initially symmetrical, with HWHM velocities of 525 km s-1. In later (t ≳ 77 days, where t is the time from outburst) spectra however, the lines displayed a distinct asymmetry, with a much stronger blue wing, possibly due to obscuration of the receding component by dust. Dust formation commenced at ˜ day 34.75 at a condensation temperature of 1480 ± 20 K, consistent with graphitic carbon. Thereafter the dust temperature declined with time as Td∝t-0.346, also consistent with graphitic carbon. The mass of dust initally rose, as a result of an increase in grain size and/or number, peaked at ˜ day 100, and then declined precipitously. This decline was most likely caused by grain shattering due to electrostatic stress after the dust was exposed to X-radiation. An Appendix summarises Planck Means for carbon, and the determination of grain mass and radius for a carbon dust shell.

  16. Predictions for signatures of the quark-nova in superluminous supernovae

    CERN Document Server

    Ouyed, Rachid; Jaikumar, Prashanth

    2009-01-01

    [Abridged] Superluminous Supernovae (SN2006gy, SN2005gj, SN2005ap, SN2008fz, SN2003ma) have been a challenge to explain by standard models. We present an alternative scenario involving a quark-nova (QN), an explosive transition of the newly born neutron star to a quark star in which a second explosion (delayed) occurs inside the already expanding ejecta of a normal SN. The reheated SN ejecta can radiate at higher levels for longer periods of time primarily due to reduced adiabatic expansion losses, unlike the standard SN case. Our model is successfully applied to SN2006gy, SN2005gj, SN2005ap, SN2008fz, SN2003ma with encouraging fits to the lightcurves. There are four predictions in our model: (i) superluminous SNe optical lightcurves should show a double-hump with the SN hump at weaker magnitudes occurring days to weeks before the QN; (ii) Two shock breakouts should be observed vis-a-vis one for a normal SN. Depending on the time delay, this would manifest as two distinct spikes in the X-ray region or a broad...

  17. Active phases and flickering of a symbiotic recurrent nova T CrB

    CERN Document Server

    Ilkiewicz, Krystian; Stoyanov, Kiril; Manousakis, Antonios; Miszalski, Brent

    2016-01-01

    T CrB is a symbiotic recurrent nova known to exhibit active phases, characterised by apparent increases in the hot component temperature and the appearance of flickering, i.e. changes in the observed flux on the time-scale of minutes. Historical UV observations have ruled out orbital variability as an explanation for flickering and instead suggest flickering is caused by variable mass transfer. We have analysed optical and X-ray observations to investigate the nature of the flickering as well as the active phases in T CrB. The spectroscopic and photometric observations confirm that the active phases follow two periods of ~1000d and ~5000d. Flickering in the X-rays is detected and follows an amplitude-flux relationship similar to that observed in the optical. The flickering is most prominent at harder X-ray energies, suggesting that it originates in the boundary layer between the accretion disc and the white dwarf. The X-ray radiation from the boundary layer is then reprocessed by a thick accretion disc or a n...

  18. Assisted stellar suicide the wind-driven evolution of the recurrent nova T Pyxidis

    CERN Document Server

    Knigge, C; Patterson, J

    2000-01-01

    We show that the extremely high luminosity of the short-period recurrent nova T Pyx in quiescence can be understood if this system is a wind-driven supersoft x-ray source (SSS). In this scenario, a strong, radiation-induced wind is excited from the secondary star and accelerates the binary evolution. The accretion rate is therefore much higher than in an ordinary cataclysmic binary at the same orbital period, as is the luminosity of the white dwarf primary. In the steady state, the enhanced luminosity is just sufficient to maintain the wind from the secondary. The accretion rate and luminosity predicted by the wind-driven model for T Pyx are in good agreement with the observational evidence. X-ray observations with Chandra or XMM may be able to confirm T Pyx's status as a SSS. T Pyx's lifetime in the wind-driven state is on the order of a million years. Its ultimate fate is not certain, but the system may very well end up destroying itself, either via the complete evaporation of the secondary star, or in a Ty...

  19. Assisted stellar suicide: the wind-driven evolution of the recurrent nova T Pyxidis

    Science.gov (United States)

    Knigge, Ch.; King, A. R.; Patterson, J.

    2000-12-01

    We show that the extremely high luminosity of the short-period recurrent nova T Pyx in quiescence can be understood if this system is a wind-driven supersoft x-ray source (SSS). In this scenario, a strong, radiation-induced wind is excited from the secondary star and accelerates the binary evolution. The accretion rate is therefore much higher than in an ordinary cataclysmic binary at the same orbital period, as is the luminosity of the white dwarf primary. In the steady state, the enhanced luminosity is just sufficient to maintain the wind from the secondary. The accretion rate and luminosity predicted by the wind-driven model for T Pyx are in good agreement with the observational evidence. X-ray observations with Chandra or XMM may be able to confirm T Pyx's status as a SSS. T Pyx's lifetime in the wind-driven state is on the order of a million years. Its ultimate fate is not certain, but the system may very well end up destroying itself, either via the complete evaporation of the secondary star, or in a Type Ia supernova if the white dwarf reaches the Chandrasekhar limit. Thus either the primary, the secondary, or both may currently be committing assisted stellar suicide.

  20. Uso da barra transpalatina no controle da rotação da mandíbula The transpalatal bar used for the mandibular rotation control

    Directory of Open Access Journals (Sweden)

    Jurandir A. Barbosa

    2005-10-01

    Full Text Available Na maioria dos pacientes na fase de dentição mista, com um certo grau de mordida aberta acompanhado de deglutição atípica ou algum mau hábito, observamos que o processo dentoalveolar superior está aumentado no sentido vertical. O uso da BTP nos molares superiores nestes casos, com a alça central colocada numa altura suficiente para, durante a deglutição, exercer alguma pressão sobre o dorso da língua, tem se mostrado de grande valia, notando-se como resultado uma restrição do crescimento do processo dentoalveolar no sentido vertical. Este resultado evita o deslocamento dentário no sentido vertical podendo até provocar movimento efetivo de intrusão dos molares com conseqüente mudança do eixo de crescimento com rotação da mandíbula no sentido anti-horário.Most of pacients in mixed dentition, with some open bite degree and atypical deglutition, we notice that the upper dentoalveolar process is increasing to the vertical side. The BTP use on the upper molar in these situations, with the central arch, low enough to make some pressure on the tongue during the deglutition. This system has been aproved as a molar intrusion movement. Can be noticed as a result the restriction of dentoalveolar process grown to the vertical side, orthopedic and jaw axes rotation grown in the horizontal direction changings.

  1. rotação intestinal em adulto, relato de caso e revisão da literatura Adult intestinal malrotation, case report and literature review

    Directory of Open Access Journals (Sweden)

    Ubirajara Rutilio Mendes e Ferreira de Araújo

    2009-12-01

    Full Text Available INTRODUÇÃO: Má rotação intestinal é entidade clínico-cirúrgica que faz parte do cotidiano do cirurgião pediátrico, mas que se torna um desafio diagnóstico quando desenvolve sintomas em adolescentes e adultos. RELATO DO CASO: Mulher deu entrada no hospital com quadro de intensa dor abdominal com três dias de evolução e piora progressiva nas últimas 24 horas. A dor apresentava piora importante após as refeições, quando era acompanhada de náuseas e vômitos. Ao exame físico apresentava-se em bom estado gera, abdômen plano, flácido, ruídos presentes, levemente doloroso à palpação de epigástrio, mas sem sinais de irritação peritoneal. Exames laboratoriais encontravam-se dentro dos limites da normalidade, bem como estudo ultrassonográfico. Não houve melhora clínica apesar do tratamento instituído e optou-se por investigação cirúrgica por tomografia sugerir má rotação intestinal. No intra-operatório observou-se todo o intestino delgado disposto para o lado direito do abdômen e o cólon para o lado esquerdo. Além disto, o jejuno proximal encontrava-se isquêmico e fazendo um volvo de 720º sobre o eixo dos vasos mesentéricos superiores. Para a correção da anomalia fez-se enterotomia do jejuno proximal, a cerca de 10 cm do ligamento de Treitz, e desconfecção do volvo, o que cursou com melhora progressiva da isquemia intestinal, permitindo que se fizesse enteroanastomose. Realizou-se ligadura do pedículo da artéria cólica média em sua origem e colectomia direita seguida de anastomose íleo-transversa látero-lateral. A paciente evolui bem. CONCLUSÃO: - A má rotação intestinal em adultos é doença de difícil diagnóstico primário, devido a não constar entre as hipóteses diagnósticas iniciais do cirurgião geral.INTRODUCTION: Intestinal malrotation is a clinical surgical entity that is present in the everyday practice of the pediatric surgeon. However, it becomes a diagnostic challenge when

  2. Radiation Therapy

    Science.gov (United States)

    ... the area is stitched shut. Another treatment, called proton-beam radiation therapy , focuses the radiation on the ... after radiation treatment ends. Sore mouth and tooth decay. If you received radiation therapy to the head ...

  3. Radiation sickness

    Science.gov (United States)

    ... radiation. There are two basic types of radiation: ionizing and nonionizing. Nonionizing radiation comes in the form of light, radio waves, microwaves and radar. This kind of radiation usually ...

  4. 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

  5. SU-E-I-33: Establishment of CT Diagnostic Reference Levels in Province Nova Scotia

    Energy Technology Data Exchange (ETDEWEB)

    Tonkopi, E; Abdolell, M; Duffy, S [Dalhousie University and Queen Elizabeth II Health Sciences Centre, Halifax, NS (Canada)

    2015-06-15

    Purpose: To evaluate patient radiation dose from the most frequently performed CT examinations and to establish provincial diagnostic reference levels (DRLs) as a tool for protocol optimization. Methods: The study investigated the following CT examinations: head, chest, abdomen/pelvis, and chest/abdomen/pelvis (CAP). Dose data, volume CT dose index (CTDIvol) and dose-length product (DLP), were collected from 15 CT scanners installed during 2004–2014 in 11 hospital sites of Nova Scotia. All scanners had dose modulation options and multislice capability (16–128 detector rows). The sample for each protocol included 15 average size patients (70±20 kg). Provincial DRLs were calculated as the 75th percentile of patient dose distributions. The differences in dose between hospitals were evaluated with a single factor ANOVA statistical test. Generalized linear modeling was used to determine the factors associated with higher radiation dose. A sample of 36 abdominal studies performed on three different scanners was blinded and randomized for an assessment by an experienced radiologist who graded the imaging quality of anatomic structures. Results: Data for 900 patients were collected. The DRLs were proposed using CTDIvol (mGy) and DLP (mGy*cm) values for CT head (67 and 1049, respectively), chest (12 and 393), abdomen/pelvis (16 and 717), and CAP (14 and 1034). These DRLs were lower than the published national data except for the head CTDIvol. The differences between the means of the dose distributions from each scanner were statistically significant (p<0.05) for all examinations. A very weak correlation was found between the dose and the scanner age or the number of slices with Pearson’s correlation coefficients of 0.011–0.315. The blinded analysis of image quality demonstrated no clinically significant difference except for the noise category. Conclusion: Provincial DRLs were established for typical CT examinations. The variations in dose between the hospitals

  6. New outburst of the symbiotic nova AG Pegasi after 165 yr

    Science.gov (United States)

    Skopal, A.; Shugarov, S. Yu.; Sekeráš, M.; Wolf, M.; Tarasova, T. N.; Teyssier, F.; Fujii, M.; Guarro, J.; Garde, O.; Graham, K.; Lester, T.; Bouttard, V.; Lemoult, T.; Sollecchia, U.; Montier, J.; Boyd, D.

    2017-08-01

    Context. AG Peg is known as the slowest symbiotic nova, which experienced its nova-like outburst around 1850. After 165 yr, during June of 2015, it erupted again showing characteristics of the Z And-type outburst. Aims: The primary objective is to determine basic characteristics, the nature and type of the 2015 outburst of AG Peg. Methods: We achieved this aim by modelling the spectral energy distribution using low-resolution spectroscopy (330-750 nm; R = 500-1000), medium-resolution spectroscopy (420-720 nm; R 11 000), and UBVRCIC photometry covering the 2015 outburst with a high cadence. Optical observations were complemented with the archival HST and FUSE spectra from the preceding quiescence. Results: During the outburst, the luminosity of the hot component was in the range of 2-11 × 1037 (d/ 0.8 kpc)2 erg s-1, being in correlation with the light curve (LC) profile. To generate the maximum luminosity by the hydrogen burning, the white dwarf (WD) had to accrete at 3 × 10-7 M⊙ yr-1, which exceeds the stable-burning limit and thus led to blowing optically thick wind from the WD. We determined its mass-loss rate to a few × 10-6 M⊙ yr-1. At the high temperature of the ionising source, 1.5-2.3 × 105 K, the wind converted a fraction of the WD's photospheric radiation into the nebular emission that dominated the optical. A one order of magnitude increase of the emission measure, from a few × 1059 (d/ 0.8 kpc)2 cm-3 during quiescence, to a few × 1060 (d/ 0.8 kpc)2 cm-3 during the outburst, caused a 2 mag brightening in the LC, which is classified as the Z And-type of the outburst. Conclusions: The very high nebular emission and the presence of a disk-like H I region encompassing the WD, as indicated by a significant broadening and high flux of the Raman-scattered O vi 6825 Å line during the outburst, is consistent with the ionisation structure of hot components in symbiotic stars during active phases. Full Table 1 and Table 6 are only available at the CDS are

  7. Radiation dosimetry.

    OpenAIRE

    Cameron, J

    1991-01-01

    This article summarizes the basic facts about the measurement of ionizing radiation, usually referred to as radiation dosimetry. The article defines the common radiation quantities and units; gives typical levels of natural radiation and medical exposures; and describes the most important biological effects of radiation and the methods used to measure radiation. Finally, a proposal is made for a new radiation risk unit to make radiation risks more understandable to nonspecialists.

  8. Rotação e sucessão de culturas para o manejo do nematoide reniforme em área de produção de soja

    Directory of Open Access Journals (Sweden)

    Hugo Márcio Leandro

    2015-06-01

    Full Text Available O nematoide reniforme (Rotylenchulus reniformis tem se tornado crescente problema fitossanitário da cultura da soja. Considerando a limitada disponibilidade de cultivares de soja que aliem resistência ao nematoide a outras características agronômicas desejáveis, estuda-se a possibilidade de utilização de manejo cultural para seu controle. Este trabalho visou avaliar o efeito da rotação de culturas no verão com milho, Crotalaria ochroleuca ou soja; e o manejo de entressafra, com Brachiaria ruziziensis como espécie de cobertura ou pousio. O experimento foi implantado em solo naturalmente infestado pelo nematoide reniforme (1245 nematoides/200cc de solo em delineamento experimental de blocos ao acaso, com quatro repetições, em esquema fatorial 3x2 (cultivos de verão x manejo de entressafra. Foram avaliadas a densidade populacional do nematoide no solo e sua variação durante as safras e entressafras, bem como a produtividade da soja na safra subsequente à rotação de culturas. Não houve efeito do manejo da entressafra com braquiária sobre o nematoide. A rotação de culturas com milho ou crotalária no verão propiciou redução da densidade populacional do nematoide reniforme em comparação ao monocultivo de soja, com reflexos positivos sobre a produtividade de soja na safra seguinte

  9. 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.

  10. 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...

  11. 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...

  12. 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.

  13. Rotação do jato em DG tau próximo à região de sua formação: análise comparativa das velocidades radiais simuladas e observadas

    Science.gov (United States)

    Cerqueira, A. H.; de Gouveia dal Pino, E. M.

    2003-08-01

    Os modelos magneto-centrífugos utilizados para explicar a formação dos jatos Herbig-Haro assumem a presença de um disco de acresção em rotação kepleriana na base de lançamento do jato. Neste cenário, o jato transmite a informação da rotação do disco para regiões distantes da fonte central, além da superfície de Alfvén, na região de colimação inicial do jato. Recentemente, Bacciotti et al. (2002, ApJ, 537, L49) obtiveram pela primeira vez uma evidência observacional de rotação em um jato HH, o jato em DG Tau, em regiões próximas da fonte central, compatível (qualitativa e quantitativamente) com o esperado a partir dos modelos magneto-centrífugos para a produção e colimação inicial de jatos HH. No presente trabalho, apresentamos mapas de velocidade radial, obtidos através de simulações numéricas tri-dimensionais SPH, para um jato com características semelhantes ao jato em DG Tau, objetivando uma comparação com os mapas de velocidade radiais obtidos por Bacciotti et al.. Nossos resultados, embora preliminares, indicam que a inclusão de efeitos como a precessão, evidenciada em DG Tau (Dougados et al. 2000, A&A, 357, L61) devem ser levadas em consideração na análise da presença de rotação não só em DG Tau mas em qualquer sistema, com o uso das velocidades radias observadas. A ausência de um grau elevado de simetria axial (quebrada, por exemplo, pela precessão do eixo do jato; ou pela presença de uma superfície interna de trabalho, ou seja, um bow shock interno), implica também em uma maior complexidade nos mapas, com conseqüências relevantes para suas interpretações.

  14. Um estudo de caso para apoio a detecção de conflitos de tráfego aéreo em rotas utilizando “detectar”

    OpenAIRE

    Cunha, Adilson Marques da; Lovato, Agnaldo Volpe

    2003-01-01

    Este artigo descreve o desenvolvimento de um Protótipo de Sistema de Software baseado na tecnologia de Ambientes Integrados de Engenharia de Software Ajudada por Computador (Integrated Computer Aided Software Engineering Environment – I-CASE-E). O Protótipo foi desenvolvido como parte de um Estudo de Caso utilizado para o Apoio a Detecção de Conflitos de Tráfego Aéreo em Rotas, e baseado nos conceitos de Comunicação, Navegação e Vigilância para o Gerenciamento do Tráfego Aéreo (Communicati...

  15. Análise crítica da rota tecnológica adotada no desenvolvimento de equipamento sinalizador de faltas para redes aéreas de distribuição de energia elétrica.

    OpenAIRE

    Fábio José de Andrade

    2012-01-01

    Um equipamento sinalizador luminoso de faltas foi desenvolvido pela Companhia Paulista de Força e Luz (CPFL) em parceria com a Escola Politécnica da USP e a empresa Expertise Engenharia Ltda., através de uma série de projetos de pesquisa incluídos no programa de pesquisa e desenvolvimento (P&D) regido pela Agência Nacional de Energia Elétrica (ANEEL) brasileira. Neste trabalho é feita uma análise crítica da rota tecnológica adotada no desenvolvimento do sinalizador de faltas, apontando detalh...

  16. 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.

  17. 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.

  18. 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...

  19. 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.

  20. 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.

  1. 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.

  2. 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.

  3. 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.

  4. 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.

  5. 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®

  6. 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.

  7. 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.

  8. 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.

  9. 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.

  10. 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.

  11. 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)

  12. Didaktisko rotaļspēļu izmantošana 3-4 gadu vecu bērnu vārdu krājuma paplašināšanā

    OpenAIRE

    2008-01-01

    Darba nosaukums: Didaktisko rotaļspēļu izmantošana 3-4 gadu vecu bērnu vārdu krājuma paplašināšanā. Darba autors: Ludmila Mališeva Darba zinātniskais vadītājs: Mag. Paed. Ineta Aizporiete Darba saturs: _72_ lpp., 20 attēli, 18 tabulas, analizēti 37 literatūras avoti. Pētījuma mērķis: Pētīt kā didaktiskā rotaļspēle ietekmē 3-4 gadu vecu bērnu vārdu krājuma paplašināšanā. Pētījuma teorētiskā daļa balstās uz Elnebijas.I., Kanepējas.R., Lieģeniece.D., Nazarovas.I., Svences.G., Zaķe...

  13. A reprodutibilidade da medida do volume endometrial por meio do VOCAL: a importância do passo de rotação The reproducibility of VOCAL endometrial volume measurement: importance of the step rotation

    Directory of Open Access Journals (Sweden)

    Wellington de Paula Martins

    2006-01-01

    Full Text Available OBJETIVOS: avaliar a reprodutibilidade intra-observador e interobservador da medida do volume endometrial utilizando ultra-sonografia tridimensional (3D e o programa VOCAL® (Virtual Organ Computer-aided AnaLysis. MÉTODOS: um bloco ultra-sonográfico 3D do endométrio foi obtido de cinco pacientes inférteis voluntárias que apresentavam diferentes volumes endometriais. Para cada bloco 3D, o volume endometrial foi calculado utilizando o modo manual em quatro diferentes passos de rotação (30º, 15º, 9º e 6º por dois diferentes observadores. Dez medidas foram obtidas para cada rotação e por cada observador. Testamos a diferença entre as médias com o one-way ANOVA e o pós-teste de Tukey e a reprodutibilidade com os coeficientes de correlação intraclasse. RESULTADOS: as medidas realizadas com passo de rotação de 30º foram associadas a médias significativamente menores em 3 das 5 pacientes. Não houve diferença entre as médias obtidas pelos passos de rotação de 15º, 9º ou 6º. Em nenhuma das avaliações foi notada diferença entre as médias obtidas pelos dois observadores. Os coeficientes de correlação intraclasse foram significativamente menores com o passo de rotação de 30º (todos abaixo de 0,984 que com os outros passos de rotação (todos acima de 0,996. CONCLUSÕES: o uso de passos de rotação de 15º ou menos apresentou medidas reprodutíveis do volume endometrial: não houve diferença significativa entre as médias obtidas pelos dois observadores, associado ao alto coeficiente de correlação intraclasse (>0,996. É recomendável o uso do passo de rotação de 15º, pois demora menos para ser obtido em comparação com 6º e 9º.PURPOSE: to determine the intraobserver and interobserver reproducibility of endometrial volume measurements using the VOCAL®-imaging program (Virtual Organ Computer-aided AnaLysis. METHODS: one three-dimensional (3-D ultrasound dataset of the endometrium was obtained from each of five

  14. Teatrālās rotaļas 5-6 gadu vecu bērnu radošās darbības veicināšanai pirmsskolā

    OpenAIRE

    2013-01-01

    Darba mērķis: teorētiski izpētīt un praktiski pamatot teatrālo rotaļu nozīmi 5-6 gadus vecu bērnu radošās darbības attīstībā. Pētījums sastāv no divām daļām – teorētiskās un praktiskās. Teorētiskajā daļā, pamatojoties uz tādu autoru pētījumiem kā R.Bebre, D.Dzintere, I.Stangaine, Ļ.Vigotskis, D.Lieģeniece, R.Kaņepēja, I.Pučure u.c., tiek zinātniski pamatota radošās darbības nozīme 5-6 gadus vecu bērnu attīstībā. Īpaša uzmanība pievērsta teatrālo rotaļu veidiem un to organizēšanas īpatnībām...

  15. 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.

  16. 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.

  17. 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.

  18. 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...

  19. 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.

  20. 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.

  1. 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.

  2. 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.

  3. 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.)

  4. 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.

  5. 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.

  6. One-step multiplex real-time RT-PCR assay for detecting and genotyping wild-type group A rotavirus strains and vaccine strains (Rotarix® and RotaTeq® in stool samples

    Directory of Open Access Journals (Sweden)

    Rashi Gautam

    2016-01-01

    Full Text Available Background. Group A rotavirus (RVA infection is the major cause of acute gastroenteritis (AGE in young children worldwide. Introduction of two live-attenuated rotavirus vaccines, RotaTeq® and Rotarix®, has dramatically reduced RVA associated AGE and mortality in developed as well as in many developing countries. High-throughput methods are needed to genotype rotavirus wild-type strains and to identify vaccine strains in stool samples. Quantitative RT-PCR assays (qRT-PCR offer several advantages including increased sensitivity, higher throughput, and faster turnaround time. Methods. In this study, a one-step multiplex qRT-PCR assay was developed to detect and genotype wild-type strains and vaccine (Rotarix® and RotaTeq® rotavirus strains along with an internal processing control (Xeno or MS2 RNA. Real-time RT-PCR assays were designed for VP7 (G1, G2, G3, G4, G9, G12 and VP4 (P[4], P[6] and P[8] genotypes. The multiplex qRT-PCR assay also included previously published NSP3 qRT-PCR for rotavirus detection and Rotarix® NSP2 and RotaTeq® VP6 qRT-PCRs for detection of Rotarix® and RotaTeq® vaccine strains respectively. The multiplex qRT-PCR assay was validated using 853 sequence confirmed stool samples and 24 lab cultured strains of different rotavirus genotypes. By using thermostable rTth polymerase enzyme, dsRNA denaturation, reverse transcription (RT and amplification (PCR steps were performed in single tube by uninterrupted thermocycling profile to reduce chances of sample cross contamination and for rapid generation of results. For quantification, standard curves were generated using dsRNA transcripts derived from RVA gene segments. Results. The VP7 qRT-PCRs exhibited 98.8–100% sensitivity, 99.7–100% specificity, 85–95% efficiency and a limit of detection of 4–60 copies per singleplex reaction. The VP7 qRT-PCRs exhibited 81–92% efficiency and limit of detection of 150–600 copies in multiplex reactions. The VP4 q

  7. One-step multiplex real-time RT-PCR assay for detecting and genotyping wild-type group A rotavirus strains and vaccine strains (Rotarix® and RotaTeq®) in stool samples.

    Science.gov (United States)

    Gautam, Rashi; Mijatovic-Rustempasic, Slavica; Esona, Mathew D; Tam, Ka Ian; Quaye, Osbourne; Bowen, Michael D

    2016-01-01

    Background. Group A rotavirus (RVA) infection is the major cause of acute gastroenteritis (AGE) in young children worldwide. Introduction of two live-attenuated rotavirus vaccines, RotaTeq® and Rotarix®, has dramatically reduced RVA associated AGE and mortality in developed as well as in many developing countries. High-throughput methods are needed to genotype rotavirus wild-type strains and to identify vaccine strains in stool samples. Quantitative RT-PCR assays (qRT-PCR) offer several advantages including increased sensitivity, higher throughput, and faster turnaround time. Methods. In this study, a one-step multiplex qRT-PCR assay was developed to detect and genotype wild-type strains and vaccine (Rotarix® and RotaTeq®) rotavirus strains along with an internal processing control (Xeno or MS2 RNA). Real-time RT-PCR assays were designed for VP7 (G1, G2, G3, G4, G9, G12) and VP4 (P[4], P[6] and P[8]) genotypes. The multiplex qRT-PCR assay also included previously published NSP3 qRT-PCR for rotavirus detection and Rotarix® NSP2 and RotaTeq® VP6 qRT-PCRs for detection of Rotarix® and RotaTeq® vaccine strains respectively. The multiplex qRT-PCR assay was validated using 853 sequence confirmed stool samples and 24 lab cultured strains of different rotavirus genotypes. By using thermostable rTth polymerase enzyme, dsRNA denaturation, reverse transcription (RT) and amplification (PCR) steps were performed in single tube by uninterrupted thermocycling profile to reduce chances of sample cross contamination and for rapid generation of results. For quantification, standard curves were generated using dsRNA transcripts derived from RVA gene segments. Results. The VP7 qRT-PCRs exhibited 98.8-100% sensitivity, 99.7-100% specificity, 85-95% efficiency and a limit of detection of 4-60 copies per singleplex reaction. The VP7 qRT-PCRs exhibited 81-92% efficiency and limit of detection of 150-600 copies in multiplex reactions. The VP4 qRT-PCRs exhibited 98

  8. Atributos físicos de um Latossolo Vermelho e produtividade de culturas cultivadas em sucessão e rotação Physical properties of an Oxisol and crops yield under succession and rotation

    Directory of Open Access Journals (Sweden)

    Silvio Aymone Genro Junior

    2009-02-01

    Full Text Available Este estudo objetivou avaliar os efeitos da sucessão e rotação de culturas nos atributos físicos e na produtividade dos cultivos agrícolas de um Latossolo Vermelho sob plantio direto, localizado no Estado do Rio Grande do Sul. Os tratamentos contaram de quatro seqüências de culturas cultivadas de 1998 a 2001: 1 sucessão trigo / soja; 2 rotação milho / aveia / milho+guandu anão / trigo / soja / trigo; 3 rotação guandu anão / trigo / soja / trigo / soja / aveia; e 4 rotação Crotalária / trigo / soja / aveia / milho / trigo. Em outubro de 2000 e de 2001, foram coletadas amostras de solo para determinar os atributos físicos do solo. Em todas as safras foi medida a produtividade das culturas. O Latossolo Vermelho cultivado com plantio direto apresenta um grau de compactação elevado, com densidade do solo acima e volume de macroporos abaixo do limite crítico para a classe textural muito argiloso. As maiores limitações ocorrem abaixo da camada de 0 a 0,03m, pois na camada mais superficial, apesar das pressões exercidas, a mobilização do solo nas operações de semeadura e adubação em linha aumenta a porosidade e reduz a densidade do solo. Nessa camada, houve maior volume de poros entre a saturação e a capacidade de campo, responsáveis pela aeração do solo, e entre a capacidade de campo e o ponto de murcha permanente, responsáveis pelo armazenamento da água disponível para as plantas. A introdução de plantas de cobertura a cada três anos não foi eficiente para reduzir a compactação. A produtividade das culturas foi influenciada positivamente na rotação com Crotalária, enquanto os demais sistemas não diferiram da sucessão de culturas.This study had as objective to evaluate the effects of crops succession and rotation on physical properties and crops yield on an Oxisol (clayey Haplortox under no tillage system, in Rio Grande do Sul State, Brazil. The treatments included four cropping sequences, used from 1998

  9. Influência da Velocidade de Rotação do Rebite na Microestrutura e no Desempenho Mecânico de Juntas de Compósito Termofixo Rebitadas por Fricção

    Directory of Open Access Journals (Sweden)

    Natascha Zocoller Borba

    2016-03-01

    Full Text Available Resumo A Rebitagem por Fricção tem se demonstrado como alternativa para união de perfis de compósito termofixo aplicados na construção civil, frente às necessidades atuais por tecnologias eficientes de união de estruturas multimateriais. Nesse processo, a extremidade de um rebite metálico é plastificada e forjada dentro de um componente polimérico, via calor friccional. Sua viabilidade técnica já foi demonstrada para juntas de Ti-6Al-4V/poliéster termofixo reforçado com fibra de vidro. Este artigo tem como objetivo complementar esse estudo através da análise do efeito da velocidade de rotação do rebite na temperatura do processo, microestrutura e propriedades mecânicas locais e globais das juntas. Foram fabricadas juntas com dois níveis de velocidade de rotação: 9000 rpm e 10000 rpm (os demais parâmetros foram mantidos constantes. Temperaturas do processo (655-765 °C superiores em 96% da temperatura de início de decomposição da matriz de poliéster (370 °C foram atingidas, desencadeando degradação polimérica acentuada na região de união. O aumento da velocidade de rotação e, portanto, do aporte térmico, não contribuiu estatisticamente para o aumento na profundidade de penetração e na largura da extremidade deformada do rebite. Porém, a extensão da área polimérica degradada aumentou em 47%, a qual resultou em redução proporcional de 50% da resistência à tração das juntas (de 4,0 ± 1,2 kN para 2,0 ± 0,7 kN. Adicionalmente, mapas de microdureza no rebite evidenciaram possíveis transformações de fase da liga que favoreceram seu endurecimento, com o aumento da velocidade de rotação. Contudo, nenhuma correlação pôde ser evidenciada entre a dureza e o desempenho mecânico das juntas sob tração, já que as amostras falharam majoritariamente por arrancamento completo do rebite da placa de compósito. Portanto, no desenvolvimento de juntas rebitadas por fricção de Ti-6Al-4V/ poli

  10. Microbial soil quality indicators under different crop rotations and tillage management Indicadores microbianos da qualidade do solo sob diferentes rotações de culturas e manejo do solo

    Directory of Open Access Journals (Sweden)

    Enderson Petrônio de Brito Ferreira

    2010-06-01

    Full Text Available An experiment was carried out under field conditions to assess the effects of soil management (no-tillage- NT and conventional tillage- CT and crop rotation systems on microbial biomass-C (Cmic, basal soil respiration (BSR, metabolic quotient (qCO2, soil organic carbon content (Corg and microbial carbon to organic carbon ratio (Cmic/Corg. Soil samples were collected on an area cultivated with wheat as winter crop and soybean as summer crop, both in rotation with vetch, maize and oats. Samples were also collected in a secondary forest used as reference. Data of each management system (NT and CT were compared to forest area by "t" test (pFoi conduzido um experimento sob condições de campo para avaliar o efeito da forma de manejo do solo (Plantio direto - PD e plantio convencional - PC e dos sistemas de rotação de culturas sobre o carbono da biomassa microbiana (Cmic, respiração basal do solo (RBS, quociente metabólico (qCO2, carbono orgânico total (Corg e relação carbono da biomassa microbiana: carbono orgânico total (Cmic/Corg. As amostras de solo foram coletadas em uma área cultivada com trigo como cultura de inverno e soja como cultura de verão, ambas em rotação com ervilhaca, milho e aveia preta. Amostras de solo também foram coletadas em uma floresta secundária usada com referência. Os dados de cada sistema de manejo do solo (PD e PC foram comparados com a floresta secundária pelo teste "t" (p<0.05 e as rotações de culturas foram comparadas pelo teste de Tukey (p<0.05. Todos os dados foram submetidos a uma análise multivariada (Análise de Componentes Principais - ACP. Foram observadas diferenças significativas (teste "t"; p<0.05 para Cmic, RBS, qCO2 e Cmic/Corg entre PD e PC, em que estes valores foram semelhantes àqueles encontrados na floresta. Entre as rotações de culturas foram observadas diferenças significativas (teste de Tukey; p<0.05 apenas para RBS e qCO2. A análise de componentes principais mostrou que o

  11. Radiation Therapy

    Science.gov (United States)

    Radiation therapy is a cancer treatment. It uses high doses of radiation to kill cancer cells and stop them from ... half of all cancer patients receive it. The radiation may be external, from special machines, or internal, ...

  12. 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 ...

  13. Stability, fragility, and Rota's Conjecture

    NARCIS (Netherlands)

    Mayhew, D.; Whittle, G.; Zwam, S.H.M. van

    2010-01-01

    Fix a matroid N. A matroid M is N-fragile if, for each element e of M, at least one of M\\e and M/e has no N-minor. The Bounded Canopy Conjecture is that all GF(q)-representable matroids M that have an N-minor and are N-fragile have branch width bounded by a constant depending only on q and N. A matr

  14. Stability, fragility, and Rota's Conjecture

    NARCIS (Netherlands)

    Mayhew, D.; Whittle, G.; Zwam, S.H.M. van

    2011-01-01

    Fix a matroid N. A matroid M is N-fragile if, for each element e of M, at least one of M\\e and M/e has no N-minor. The Bounded Canopy Conjecture is that all GF(q)-representable matroids M that have an N-minor and are N-fragile have branch width bounded by a constant depending only on q and N. A matr

  15. 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...

  16. 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.

  17. 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 ...

  18. 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.

  19. Radiation dosimetry

    CERN Document Server

    Hine, Gerald J; Hine, Gerald J

    1956-01-01

    Radiation Dosimetry focuses on the advancements, processes, technologies, techniques, and principles involved in radiation dosimetry, including counters and calibration and standardization techniques. The selection first offers information on radiation units and the theory of ionization dosimetry and interaction of radiation with matter. Topics include quantities derivable from roentgens, determination of dose in roentgens, ionization dosimetry of high-energy photons and corpuscular radiations, and heavy charged particles. The text then examines the biological and medical effects of radiation,

  20. 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.

  1. 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.

  2. 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.

  3. 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.

  4. 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.

  5. 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...

  6. 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...

  7. 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 ...

  8. 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.

  9. 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.

  10. 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.

  11. 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).

  12. 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 ...

  13. 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.

  14. 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.

  15. 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

  16. Safety of the pentavalent rotavirus vaccine (PRV), RotaTeq(®), in Kenya, including among HIV-infected and HIV-exposed infants.

    Science.gov (United States)

    Laserson, Kayla F; Nyakundi, Daveline; Feikin, Daniel R; Nyambane, Geoffrey; Cook, Earnest; Oyieko, Janet; Ojwando, Joel; Rivers, Stephen B; Ciarlet, Max; Neuzil, Kathleen M; Breiman, Robert F

    2012-04-27

    Two multicenter Phase III trials were conducted in five countries from March 2007 to March 2009 to evaluate the safety and efficacy of the pentavalent rotavirus vaccine (PRV), RotaTeq(®), in Africa and Asia. In this report, we evaluate the safety of this vaccine, including among HIV-infected and HIV-exposed infants, in Kenya. 1308 Infants were randomized 1:1 to receive 3 doses of PRV/placebo at approximately 6, 10, and 14 weeks of age. HIV counseling and testing were offered to all participants. A positive PCR result indicated HIV infection; the presence of HIV antibody in PCR-negative children indicated HIV exposure without HIV infection. All serious adverse events (SAE) within 14 days of any dose, and vaccine-related SAEs, intussusception, and deaths occurring at any time during the study, were reported ("SAE surveillance"). In addition, 297 participants were followed for 42 days after any dose for any adverse event (AE), regardless of severity ("intensive safety surveillance"). The safety evaluation was stratified by HIV status. SAEs were reported in 20/649 vaccine recipients (3.1%) and 21/643 placebo recipients (3.3%) within 14 days following vaccination (p = 0.9). The most common SAE in the vaccinated group was pneumonia (1.7%). No individual SAE was significantly more common among vaccine vs. placebo recipients. Seventy-two deaths were reported, 38 (5.9%) and 34 (5.3%) among vaccine and placebo recipients, respectively (p = 0.66). No cases of intussusception were reported. During intensive safety surveillance, 137/147 (93.2%) vaccine recipients and 147/150 (98.0%) placebo recipients experienced one or more AEs (risk ratio = 0.95; 95% CI: 0.91-1.0; p = 0.05). 88.5% of the infants were tested for HIV infection; 21/581 (3.6%) children in the vaccine group and 17/577 (2.9%) in the placebo group were HIV-infected. Among the 37 HIV-infected infants with full safety follow-up, 5/21 (23.8%) vaccine recipients and 2/16 (12.5%) placebo recipients reported an SAE (p

  17. Radiation protection

    CERN Document Server

    CERN. Geneva

    2001-01-01

    This will be a simple explanation of the reasons why CERN has to be careful about radiation protections issues, a practical guide on how to recognize radiation dangers, the monitoring systems that make sure radiation levels are well tolerable norms, and a quick summary of what radiation levels mean in terms of personal risk.

  18. Nota biobibliográfica + poética + creaciones («Uves migratorias», «Fronteras del hambre», «Puntos de sutura», «Paisaje urbano 2», «El intruso» y «Mirada rota» + cuestionario (Victoria Pineda

    Directory of Open Access Journals (Sweden)

    Julián Alonso

    2014-03-01

    Full Text Available Nota biobibliográfica + poética + creaciones («Uves migratorias», «Fronteras del hambre», «Puntos de sutura», «Paisaje urbano 2», «El intruso» y «Mirada rota» + cuestionario (Victoria Pineda

  19. Isotopic 32S/33S ratio as a diagnostic of presolar grains from novae

    Directory of Open Access Journals (Sweden)

    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.

  20. 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.

  1. Caminhos atlânticos memória, patrimônio e representações da escravidão na Rota dos Escravos Atlantic routes memory, heritage and slave representations on the Slave Route

    Directory of Open Access Journals (Sweden)

    Ana Lucia Araújo

    2009-06-01

    Full Text Available O artigo examina as diferentes representações da escravidão e do tráfico atlântico presentes na Rota dos Escravos da cidade de Ajudá, na atual República do Benim. Busca-se entender como estas representações exprimem e reconstroem diferentes memórias do passado escravista atlântico. Tenta-se mostrar que a Rota dos Escravos é um lugar construído, onde se percebem duas imagens do escravo, a da vítima absoluta e a do resistente. O percurso proposto sugere dois níveis de leitura: de um lado, os monumentos constituem uma encenação, cujo objetivo é emocionar os descendentes da diáspora (principalmente os norteamericanos, que têm recursos financeiros para fazer turismo em países estrangeiros; de outro lado, as estátuas concebidas pelo artista Cyprien Tokoudagaba e os templos existentes na Rota dos Escravos posicionam o visitante no cruzamento de diferentes memórias e diferentes histórias da escravidão, onde a vitimização dá lugar à afirmação cultural que valoriza a arte, as religiões e as culturas africanas.This paper examines the different representations of slavery and the slave trade found on the Slaves Route in Ouidah, present Republic of Benin. It aims at understanding how these representations express and reconstruct different memories of the Atlantic slave past. The paper shows that Ouidah's Slaves Route is a constructed space, where we can find two different images of enslaved Africans: the absolute victim and the resister. The proposed itinerary suggests two levels of interpretation: on the one hand, the monuments staging the past aim at emotionally move the diaspora (especially African Americans who have the financial resources to travel abroad; on the other hand, the statues conceived by Cyprien Tokoudagaba and the existing vodun temples on the Slaves Route place the visitor at the crossing position between different memories and different histories of slavery, where victimization is replaced by cultural

  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. 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...

  11. 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.

  12. 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 ...

  13. 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.

  14. 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...

  15. Dietilamida do ácido lisérgico (LSD) e N,N-dimetiltriptamina (DMT) como substratos de peroxidases: uma possível rota de metabolização

    OpenAIRE

    Melissa Medrano Gomes

    2008-01-01

    Após um intervalo de duas décadas, ressurgiu um novo interesse em estudos sobre alucinógenos que visam a compreensão de como estes compostos interagem com o sistema nervoso central (SNC). Sabendo-se que enzimas do tipo peroxidases estão presentes em células do tipo leucócitos, neurônios e microglia, e que, são capazes de oxidar compostos indólicos, esta, portanto, poderia representar uma rota ativa de metabolização de alucinógenos no SNC, ainda não conhecida. Nesta perspectiva, este trabalho ...

  16. Neumotórax y bulla enfisematosa gigante rota como manifestación inicial de un carcinoma Pneumothorax and ruptured giant emphysematous bulla as a manifestation of carcinoma

    OpenAIRE

    Orestes Noel Mederos Curbelo; Juan Carlos Barrera Ortega; Evelio Guerra Pereda; José Manuel Da Costa Fernández

    2010-01-01

    Se presenta el caso de un paciente de 64 años de edad que acudió al cuerpo de guardia con dolor torácico agudo localizado en hemitórax derecho y disnea intensa. La persistencia del neumotórax sin que se lograra la reexpansión pulmonar con la pleurotomía y el drenaje torácico obligó a una toracotomía. Se encontró una bulla enfisematosa gigante rota, y se realizó una bilobectomía superior y media. El diagnóstico histológico fue carcinoma bronquioalveolar. La coincidencia de un cáncer de pulmón ...

  17. Influência da manipulação osteopática na amplitude de rotação da coluna cervical em indivíduos com cervicalgia mecânica crônica

    OpenAIRE

    Stelle,Rafael; Zeigelboim, Bianca Simone; Lange, Marcos Christiano; Marques, Jair Mendes, 1947-

    2013-01-01

    JUSTIFICATIVA E OBJETIVOS: A amplitude de movimento do pescoço pode ser reduzida pela presença de disfunções vertebrais e miofasciais, as quais podem ser tratadas pela manipulação osteopática por meio da técnica articulatória rítmica cervical. O objetivo deste estudo foi verificar se a manipulação osteopática, através da técnica articulatória rítmica gera aumento da amplitude de rotação cervical mensurada por fleximetria. MÉTODOS: A casuística foi constituída de 58 indivíduos de ambos os gêne...

  18. Dietilamida do ácido lisérgico (LSD) e N,N-dimetiltriptamina (DMT) como substratos de peroxidases: uma possível rota de metabolização

    OpenAIRE

    Melissa Medrano Gomes

    2008-01-01

    Após um intervalo de duas décadas, ressurgiu um novo interesse em estudos sobre alucinógenos que visam a compreensão de como estes compostos interagem com o sistema nervoso central (SNC). Sabendo-se que enzimas do tipo peroxidases estão presentes em células do tipo leucócitos, neurônios e microglia, e que, são capazes de oxidar compostos indólicos, esta, portanto, poderia representar uma rota ativa de metabolização de alucinógenos no SNC, ainda não conhecida. Nesta perspectiva, este trabalho ...

  19. Adubação Fosfatada para Alta Produtividade de Soja, Milho e Cereais de Inverno Cultivados em Rotação em Latossolos em Plantio Direto no Centro-Sul do Paraná

    Directory of Open Access Journals (Sweden)

    Renan Costa Beber Vieira

    2015-06-01

    Full Text Available O Estado do Paraná não dispõe de um sistema de recomendação de adubação para rotação de culturas em plantio direto (PD. Em razão disso, utiliza indicações geradas para culturas individuais há mais de 30 anos e em preparo convencional. Este estudo teve como objetivo consolidar a calibração de P e avaliar a resposta das culturas à adubação fosfatada, visando à proposição de um sistema de indicações técnicas para a adubação fosfatada das culturas da soja, do milho, do trigo e da cevada cultivadas em sistema de rotação em Latossolos com longo histórico de PD (>30 anos na região centro-sul do Paraná, que se caracteriza por possuir alto potencial produtivo. Três experimentos de calibração foram conduzidos de 2008 a 2013 e consistiram na criação de níveis de P pela aplicação de doses a lanço de até 640 kg ha-1 de P2O5. Quarenta e quatro experimentos de resposta a P foram conduzidos entre as safras de 2011 a 2012/13, tendo como foco avaliar a resposta das culturas a P em solos com distinta disponibilidade do nutriente. Os rendimentos relativos [RR = (rendimento sem P/rendimento máximo × 100] das culturas e os teores de P no solo (Mehlich-1 foram relacionados, obtendo-se os teores críticos e as classes de disponibilidade de P no solo. Para a estimativa das doses nas classes de disponibilidade Baixa e Média, foram utilizadas as curvas de resposta à adubação de P, seguindo a filosofia de suficiência (adubação de cultura. Nas classes de disponibilidade Alta e Muito Alta, as doses foram com base na exportação pelos grãos. Os cereais de inverno se evidenciaram mais exigentes e determinaram o teor crítico de P de 8 mg dm-3 para a rotação de culturas, considerando a camada de 0-20 cm. As doses de P indicadas para soja, milho, trigo e cevada em solos em PD de longa duração são superiores às de adubação atualmente indicadas no PR, o que, ao menos em parte, justificam-se pelas altas produtividades das

  20. The confluence zone of the intense katabatic winds at Terra Nova Bay, Antarctica, as derived from airborne sastrugi surveys and mesoscale numerical modeling

    Science.gov (United States)

    Bromwich, David H.; Parish, Thomas R.; Zorman, Christian A.

    1990-04-01

    The surface wind field inland of the intense coastal katabatic wind regime at Terra Nova Bay, Antarctica, has been studied both observationally and numerically. Airborne surveys of wind-induced features on the snow surface have been used to construct the time-averaged winter surface airflow pattern. The surface motion field has also been simulated by a mesoscale primitive equation model using terrain slopes with a horizontal resolution of 32 km. Both methods of analysis demonstrate that the intense katabatic airstream at Terra Nova Bay is forced by converging air currents in the continental interior. The broadscale confluence zone becomes organized ito tow regions within about 180 km of the coast. The primary route for katabatic mass transport into the Terra Nova Bay area is Reeves Glacier valley, but an important secondary source is provided by airflow down David Glacier. The former is generated by the Coriolis-induced concentration of mass transport on the left side (looking downwind) of the broadscale confluence zone as well as by the near-coastal mountain deflection of airflow into the valley head. The confluence zone feeding into David Glacier valley stretches over 100 km into the interior and is forced by the broadscale terrain configuration of the ice sheet. Source areas for the two airstreams differ with Reeves Glacier valley being fed by cold air formed well into the interior, whereas the airflow down David Glacier is sustained by radiative cooling over lower parts of the ice sheet which are much closer to the Ross Sea. Evaluation of the observational and modeling results reveals both the strengths and weaknesses of each approach. Airborne surveys of sastrugi orientations are a highly successful method for establishing the detailed pattern of surface airflow. However, a systematic examination of sastrugi dimensions suggests that such work could also be carried out using SPOT-type satellite observations, which is a more cost-effective approach than aircraft

  1. Radiation Therapy: Professions in Radiation Therapy

    Science.gov (United States)

    ... Resources Professions Site Index A-Z Professions in Radiation Therapy Radiation Oncologist Therapeutic Medical Physicist Radiation Therapist Dosimetrist Radiation Oncology Nurse Social Worker Dietitian Radiation Oncologist Radiation oncologists are physicians who oversee the ...

  2. Novas Fontes, Novas Versões: Contribuições do Acervo da Comissão Nacional da Verdade

    Directory of Open Access Journals (Sweden)

    Alessandra Sá Mello Costa

    2017-03-01

    Full Text Available Na área de estudos organizacionais, o interesse dos pesquisadores em utilizar fontes e acervos históricos em suas pesquisas cresce a cada dia (Rowlinson, Hassard, & Decker, 2014; Yates, 2014. Como forma de enriquecer e aprofundar a discussão sobre esse movimento, a presente pesquisa tem por objetivo refletir sobre possíveis contribuições das fontes reunidas, sistematizadas e produzidas pela Comissão Nacional da Verdade (CNV. Instituída para investigar as graves violações dos direitos humanos cometidas no regime da ditadura civil-militar brasileira, a CNV (a partir de seu acervo oferece aos pesquisadores das organizações novas versões dos fatos históricos, o que torna possível não só problematizar e rever versões históricas oficiais hegemônicas, mas também investigar fenômenos organizacionais sob outras perspectivas. Assim, após a descrição do processo de constituição e de composição do seu acervo documental, foram elencadas quatro avenidas de pesquisas iniciais: (a sobre o apoio e a participação da sociedade civil na constituição e manutenção do governo civil-militar brasileiro; (b sobre a formação de redes de agentes sociais envolvidos no processo de criação e de trabalho da CNV; (c sobre as relações de trabalho durante o período, como a atuação dos sindicatos ou as práticas de recursos humanos sob um regime autoritário; e (d sobre o tema da história e memória das empresas.

  3. On the narrow emission line components of the LMC novae 2004 (YY Dor) and 2009a

    CERN Document Server

    Mason, Elena

    2014-01-01

    We present early decline spectra of the two Large Magellanic Cloud novae: LMC 2004 (YY Dor) and LMC 2009a and discuss their spectral an line profile evolution with special emphasis on the existence and appearance of a sharp component. We show that the narrow component that characterizes the emission lines in the maximum spectra of nova LMC 2004 originates in the ejecta. The HeII 4686 A, narrow emission which appears at the onset of the nebular phase in both novae is somewhat controversial. Our observations suggest that the corresponding line forming region is physically separated from the rest of the ejecta (the broad line region) and environmentally different. However, the lack of late time observations covering the super-soft source (SSS) phase, the post-SSS phase and the quiescence state does not allow to securely establish any non-ejecta origin/contribution as, instead, in the case of U Sco and KT Eri.

  4. Expanding Pharmacists' Scope of Practice to Include Immunization in Nova Scotia

    Directory of Open Access Journals (Sweden)

    Beth O'Reilly

    2017-07-01

    Full Text Available On 10 December 2010 An Act to Amend Chapter 36 of the Acts of 2001, the Pharmacy Act (Bill 7 received Royal Assent in Nova Scotia, including an amendment that enabled an expanded scope of pharmacy practice. Expanding pharmacists' scope of practice came about from recommendations by various federal and provincial government bodies as an attempt to improve accessibility to health care and decrease costs. In 2013, pharmacists in Nova Scotia began administering the influenza vaccine as part of the publicly funded program in attempts to improve vaccine coverage rates. Preliminary evaluation in Nova Scotia has shown an increase in influenza vaccination coverage. Although pharmacist administration of influenza vaccination may improve vaccination coverage and reduce demand on physician time, there may be tension created among the professions, which needs to be addressed and managed.

  5. Superoutburst of a New Sub-Period-Minimum Dwarf Nova CSS130418 in Hercules

    Directory of Open Access Journals (Sweden)

    D. Chochol

    2015-02-01

    Full Text Available Multicolour photometry of a new dwarf nova CSS130418 in Hercules, which underwent superoutburst on April 18, 2013, allow to classified it as a WZ Sge-type dwarf nova. The phase light curves for different stages of superoutburst are presented. The early superhumps were used to determine the orbital period Porb = 64.84(1 minutes, which is shorter than the period minimum ~78 minutes for normal hydrogen-rich cataclysmic variables. We found the mean period of ordinary superhumps Psh = 65.559(1 minutes. The quiescent spectrum is rich in helium, showing double peaked emissionlines of H I and He I from accretion disk, so the dwarf nova is in a late stage of stellar evolution.

  6. The Effects of Thermonuclear Reaction Rate Variations on Nova Nucleosynthesis A Sensitivity Study

    CERN Document Server

    Iliadis, C; José, J; Starrfield, S; Tupper, P; Iliadis, Christian; Champagne, Art; Jose, Jordi; Starrfield, Sumner; Tupper, Paul

    2002-01-01

    We investigate the effects of thermonuclear reaction rate uncertainties on nova nucleosynthesis. One-zone nucleosynthesis calculations have been performed by adopting temperature-density-time profiles of the hottest hydrogen-burning zone (i.e., the region in which most of the nucleosynthesis takes place). We obtain our profiles from 7 different, recently published, hydrodynamic nova simulations covering peak temperatures in the range from Tpeak=0.145-0.418 GK. For each of these profiles, we individually varied the rates of 175 reactions within their associated errors and analyzed the resulting abundance changes of 142 isotopes in the mass range below A=40. In total, we performed 7350 nuclear reaction network calculations. We use the most recent thermonuclear reaction rate evaluations for the mass ranges A=1-20 and A=20-40. For the theoretical astrophysicist, our results indicate the extent to which nova nucleosynthesis calculations depend on presently uncertain nuclear physics input, while for the experimenta...

  7. Modelling the synchrotron light curves in recurrent novae V745 Scorpii and RS Ophiuchi

    CERN Document Server

    Kantharia, N G; Roy, N; Anupama, G C; Chitale, A; Ishwara-Chandra, C; Prabhu, T P; Ashok, N M; Banerjee, D P K

    2015-01-01

    In this paper, we present the synchrotron light curve at 610 MHz from the recurrent nova V745 Sco following its outburst on 6 February 2014. The system has been detected and periodically monitored with the Giant Metrewave Radio Telescope (GMRT) since 9 February 2014 as part of the Galactic Nova with GMRT (GNovaG) project. The light curves are well fit by a model of synchrotron emitting region obscured by foreground thermal gas which eventually becomes optically thin to the low GMRT frequencies. We present the model fit to the 2014 data on V745 Sco and discuss it alongwith the model fit to the 1.4 GHz data of the recurrent nova RS Ophiuchi following its outburst in 1985.

  8. A Far Ultraviolet Spectroscopic Analysis of the Old Nova Q Cygni

    Science.gov (United States)

    Kolobow, Craig; Sion, E. M.

    2011-01-01

    Q Cygni (Nova Cygni 1876) is one of the oldest old novae with a long orbital period of 10.08 hours and spectroscopic peculiarities in the optical including the presence of variable wind outflow revealed by optical P Cygni profiles in the He I lines and Halpha (Kafka et al.2003). There has never been a far UV spectroscopic analysis of this system. Therefore, we have carried out a synthetic spectral analysis of a far ultraviolet IUE archival spectrum of Q Cygni using our optically thick, steady state, accretion disk models and model white dwarf photospheres. We report the results of our spectroscopic analysis and compare the physical parameters we derive with those of other old novae. We gratefully acknowledge the support of this by NSF grant 0807892 to Villanova University.

  9. A bossa nova e a influência do blues, 1955-1964

    Directory of Open Access Journals (Sweden)

    Bryan McCann

    2010-06-01

    Full Text Available Este artigo considera as conexões entre blues e bossa nova, pouco reconhecidas na literatura sobre bossa nova mas muito importantes para o desenvolvimento do estilo. Analisando as gravações do circuito samba-jazz em Copacabana nas décadas de 1950 e 1960, o artigo traz à luz uma prática de blues, tanto na estrutura de doze compassos como na utilização da escala blues como matéria de improviso, bastante comum naquela época. O artigo explica o papel de figuras-chaves como Booker Pittman, Moacir Santos e Paulo Moura na transmissão de uma influência do blues no Rio de Janeiro e os efeitos dessa influência na bossa nova.

  10. Disks, Winds, and Veiling Curtains: Dissecting the Ultraviolet Spectrum of the Dwarf Nova Z Camelopardalis in Outburst

    Science.gov (United States)

    Knigge, Christian; Long, Knox S.; Blair, William P.; Wade, Richard A.

    1997-02-01

    We present a far-ultraviolet spectrum of the dwarf nova Z Cam near the peak of a normal outburst as observed with the Hopkins Ultraviolet Telescope (HUT) on the Astro-2 mission. The continuum shape and luminosity are almost identical to an Astro-1 HUT spectrum of the same object in a similar state obtained about 4 years or 50 outburst episodes earlier. This suggests that, following the onset of an outburst, the system quickly reaches a (quasi-) steady state that is insensitive to the interoutburst history. A variance analysis of the Astro-2 data reveals no evidence for spectral variability on a timescale of minutes. The rms amplitude of any intrinsic fluctuations is ignored--or that the standard picture itself may require modification. Blackbody disk models actually match the data better at longer HUT wavelengths, but the redder color of these models is a direct consequence of the neglect of all radiative transfer effects. The same neglect prevents blackbody models from reproducing the turnover in the spectrum and causes them to overpredict the accretion rate. We use a Monte Carlo line profile synthesis code to model five of the high-ionization lines in Z Cam's spectrum in terms of a simple, kinematic description of a rotating, biconical accretion disk wind. Adopting the picture of such an outflow that has recently been proposed for another cataclysmic variable, UX UMa, we find that acceptable fits to the data can be obtained. The relative mean ionization fractions we derive for the ionic species included in our wind modeling appear to be consistent with photoionization by a radiation field with T ~ 1.2 × 105 K. This temperature is within the range that has recently been inferred for Z Cam's soft X-ray component from ROSAT data and similar to the boundary layer temperature that has been derived on the basis of Extreme-Ultraviolet Explorer (EUVE) observations for the dwarf nova U Gem in outburst. An important feature of our adopted outflow model is the existence of

  11. Near-infrared studies of V2944 Ophiuchi (Nova Ophiuchi 2015)

    Science.gov (United States)

    Srivastava, Mudit K.; Banerjee, D. P. K.; Ashok, N. M.; Venkataraman, V.; Sand, D.; Diamond, T.

    2016-10-01

    We present multi-epoch near-infrared observations of Nova Ophiuchi 2015 which was discovered during outburst in March 2015. This nova showed a few special properties viz. (i) it displayed an unusual prolonged flat-top light curve which does not easily fit into known classes of nova light curves, (ii) it showed evidence for possessing an evolved secondary in the outbursting binary system, and (iii) it made a rare reverse hybrid transition from the He/N class to Fe II class early during its outburst. The present studies focus on the spectroscopic evolution of the object around maximum light and early decline. We show that there was a unique, rapid strengthening and decline in the He 1.0831, 2.0581 μm line strengths during this stage, wherein the nova combined the traits of both the He/N and Fe II classes. Possible causes for this behaviour are discussed. The relative strengths of the Lyβ fluoresced O I 0.8446, 1.1287 μm lines are used to estimate the reddening to the nova. A recombination Case B analysis of the early spectra is used to set constraints on the electron density and emission measure, and a later time spectrum when the ejecta were optically thin is used to estimate the ejecta mass to be (0.95-1.9) × 10-4 M⊙. Power-law fits made to study the evolution of the continuum, show a fairly constant slope which differs from the trend generally expected during a nova's evolution viz. beginning with a blackbody and evolving to a free-free distribution at later stages.

  12. VizieR Online Data Catalog: New Dwarf novae in SDSS, GALEX and astrom. cat. (Wils+, 2010)

    Science.gov (United States)

    Wils, P.; Gansicke, B. T.; Drake, A. J.; Southworth, J.

    2015-07-01

    Here, we cross-match a number of large surveys to find faint outbursting dwarf novae, and make use of CRTS light curves to compare the properties of the previously known dwarf novae, those identified spectroscopically by SDSS, and the ones discovered in this paper. (3 data files).

  13. Four unusual novae observed in Torun: V2362 Cyg, V2467 Cyg, V458 Vul, V2491 Cyg

    CERN Document Server

    Ragan, E; Tomov, T; Dimitrow, W; Fagas, M; Kwiatkowski, T; Schwarzenberg-Czerny, A; Buil, Ch; Swierczynski, E; Brozek, T; Cikala, M; Czart, K; Fidos, A; Frackowiak, S; Galan, C; Karska, A; Klosinska, M; Lewandowski, M; Radomski, T; Rozanski, P; Wiecek, M; Wychudzki, P; Zajczyk, A; Zielinska, M

    2010-01-01

    We present photometric and spectral observation for four novae: V2362 Cyg, V2467 Cyg, V458 Vul, V2491 Cyg. All objects belongs to the "fast novae" class. For these stars we observed different departures from a typical behavior in the light curve and spectrum.

  14. Modelling sea ice formation in the Terra Nova Bay polynya

    Science.gov (United States)

    Sansiviero, M.; Morales Maqueda, M. Á.; Fusco, G.; Aulicino, G.; Flocco, D.; Budillon, G.

    2017-02-01

    Antarctic sea ice is constantly exported from the shore by strong near surface winds that open leads and large polynyas in the pack ice. The latter, known as wind-driven polynyas, are responsible for significant water mass modification due to the high salt flux into the ocean associated with enhanced ice growth. In this article, we focus on the wind-driven Terra Nova Bay (TNB) polynya, in the western Ross Sea. Brine rejected during sea ice formation processes that occur in the TNB polynya densifies the water column leading to the formation of the most characteristic water mass of the Ross Sea, the High Salinity Shelf Water (HSSW). This water mass, in turn, takes part in the formation of Antarctic Bottom Water (AABW), the densest water mass of the world ocean, which plays a major role in the global meridional overturning circulation, thus affecting the global climate system. A simple coupled sea ice-ocean model has been developed to simulate the seasonal cycle of sea ice formation and export within a polynya. The sea ice model accounts for both thermal and mechanical ice processes. The oceanic circulation is described by a one-and-a-half layer, reduced gravity model. The domain resolution is 1 km × 1 km, which is sufficient to represent the salient features of the coastline geometry, notably the Drygalski Ice Tongue. The model is forced by a combination of Era Interim reanalysis and in-situ data from automatic weather stations, and also by a climatological oceanic dataset developed from in situ hydrographic observations. The sensitivity of the polynya to the atmospheric forcing is well reproduced by the model when atmospheric in situ measurements are combined with reanalysis data. Merging the two datasets allows us to capture in detail the strength and the spatial distribution of the katabatic winds that often drive the opening of the polynya. The model resolves fairly accurately the sea ice drift and sea ice production rates in the TNB polynya, leading to

  15. Ciencias contábeis, novos rumos , novas diretrizes curriculares

    Directory of Open Access Journals (Sweden)

    Patricia Dantas Trajano

    2009-09-01

    Full Text Available A nova Lei de Diretrizes e Bases da Educação Nacional, Lei n"9.394, de 20 de dezembro de 1996, em seu artigo 43, enfatiza que a educação superior tem por finalidade precípua a formação de profissionais aptos para inserção no mercado de trabalho e em condições de participarem ativamente do desenvolvimento da sociedade brasileira. Prevê, ainda, o incentivo a pesquisa, a educação continuada, assim como a promoção da divulgação de conhecimentos culturais, científicos e técnicos que constituam patrimônio da humanidade. O inciso II do artigo 53 da mesma Lei concede autonomia as Instituições de Ensino Superior (IES para "fixar os currículos dos seus cursos e programas, observadas as diretrizes gerais pertinentes", o que oferece as IES uma maior flexibilidade na elaboração de seu currículo pleno. A Resolução n2 03/92, do Conselho Federal de Educação, fixa, ate o momento, os mínimos de conteúdo e de duração do curso de graduação em Ciências Contábeis vigentes no pals. Estabelece que o currículo pleno das IES deva definir o perfil profissional a ser formado, em função das atribuições legais que lhe serão conferidas, das peculiaridades e necessidades da região em que as IES se encontram, de suas naturezas e características próprias. O currículo pleno deve ser dividido por disciplinas ou outras atividades curriculares obrigatórias eletivas, nas seguintes categorias de conhecimentos: Categoria I - Conhecimentos de Formação Geral de natureza humanística e social; Categoria II - Conhecimentos de Formação Profissional; Categoria III - Conhecimentos ou Atividades de Formação.

  16. ENSINO MÉDIO ARTICULADO AO ENSINO PROFISSIONALIZANTE: NOVAS PERSPECTIVAS

    Directory of Open Access Journals (Sweden)

    S. H. S. L. M. Freire

    2012-05-01

    Full Text Available Neste artigo pretendemos discutir sobre a nova proposta do Ensino Médio articulado ao Ensino profissionalizante, nas instituições SESI e SENAI na cidade de Mossoró/RN. Essa proposta tem por finalidade proporcionar a formação integral, alicerçada nas dimensões do trabalho, ciência e cultura e ampliar as possibilidades de inserção do cidadão na vida produtiva e social, bem como dar continuidade ao seu itinerário formativo, contribuindo para a formação continuada e permanente do aluno. Dessa maneira, objetivamos com esse estudo analisar as contribuições dessa articulação para ensino - aprendizagem do aluno e as possibilidades de construção de novos conhecimentos. O estudo fundamenta-se em documentos como referenciais normativos, pedagógico, operacionais e financeiros nacionais para a articulação da educação básica do SESI com a educação profissional do SENAI (2006, relatório de mapeamento e diagnóstico do Projeto EBEP, Educação básica do SESI articulada com educação Profissional do SENAI (2001; 2011. A ênfase dada pela LDB (Lei de Diretrizes e Bases da Educação 9.394/96, para a educação profissional deixa claro que deve ser desenvolvida em articulação com o ensino regular ou por diferentes estratégias de educação continuada numa perspectiva do exercício pleno da cidadania. Esta pesquisa é resultado de um trabalho exploratório-bibliográfico que tem como objetivo maior compreender as reflexões e proposições atribuídas a essa articulação médio com o ensino profissionalizante na contemporaneidade.

  17. Johannes Kepler and David Fabricius: Their Discussion on the Nova of 1604

    Science.gov (United States)

    Granada, Miguel A.

    David Fabricius (1564-1617) was one of the most important astronomers in the period between 1596, the year of publication of Kepler's Mysterium cosmographicum, and 1609, the year of publication of the Astronomia nova.1 Kepler praised Fabricius as the most accurate observational astronomer after Tycho Brahe's death in 1601.2 Fabricius was a Reformed pastor in Ostfriesland (East Frisia), his remote natal region, and a vocational astronomer. He published nothing in the field of astronomy except for the short treatises between 1604 and 1606 concerning the nova that appeared in October 1604 in Serpentarius.

  18. High energy emission of symbiotic recurrent novae: RS Ophiuchi and V407 Cygni

    CERN Document Server

    Hernanz, Margarita

    2011-01-01

    Recurrent novae occurring in symbiotic binaries are candidate sources of high energy photons, reaching GeV energies. Such emission is a consequence of particle acceleration leading to pion production. The shock between matter ejected by the white dwarf, undergoing a nova explosion, and the wind from the red giant companion is responsible for such a process, which mimics a supernova remnant but with much smaller energetic output and much shorter time scales. Inverse Compton can also be responsible for high energy emission. Recent examples are V407 Cyg, detected by Fermi, and RS Oph, which unfortunately exploded in 2006, before Fermi was launched.

  19. As novas formas de controle em One Dimensional Man, de Herbert Marcuse

    OpenAIRE

    Jannarelli, Vicente Claudio

    2010-01-01

    One-Dimensional Man trabalha com certas tendências básicas da sociedade industrial avançada que parecem indicar uma nova fase de civilização. Tais tendências geraram uma forma de pensamento e comportamento que minou a base da cultura tradicional. A principal característica dessa nova forma de pensamento e de comportamento é a repressão de todos os valores, aspirações, e idéias que não podem ser definidas em termos de operações e atitudes validadas pelas formas prevalecentes de racionalidade. ...

  20. Study of the Quasi-Elastic Scattering in the NOvA Detector Prototype

    Energy Technology Data Exchange (ETDEWEB)

    Betancourt, Minerba [Univ. of Minnesota, Minneapolis, MN (United States)

    2013-06-01

    NOvA is a 810 km long base-line neutrino oscillation experiment with two detectors (far 14 KTon and near detector 300 Ton) currently being installed in the NUMI o -axis neutrino beam produced at Fermilab. A 222 Ton prototype NOvA detector (NDOS) was built and operated in the neutrino beam for over a year to understand the response of the detector and its construction. The goal of this thesis is to study the muon neutrino interaction data collected in this test, specifically the identification of quasi-elastic charged-current interactions and measure the behavior of the quasi-elastic muon neutrino cross section.

  1. Clio e outras tramas: a nova história cultural e a literatura comparada

    OpenAIRE

    Martins, Ricardo André Ferreira

    2012-01-01

    A “História Cultural” e a “Nova História Cultural” são linhas de reflexão teórica e metodológica que podem oferecer aos estudos em Literatura Comparada novos horizontes e limites interdisciplinares que resultariam na abertura para novos campos de pesquisas comparatistas. A abordagem cultural, na medida em que ela se encontra nas práticas de investigação comparatistas, permitiria ao estudioso ou pesquisador em Literatura Comparada cotejar não somente novos objetos de estudos, mas também novas ...

  2. Fermi-LAT Gamma-ray Observations of Nova Lupus 2016 (ASASSN-16kt)

    Science.gov (United States)

    Cheung, C. C.; Jean, P.; Shore, S. N.; Fermi Large Area Telescope Collaboration

    2016-10-01

    The Fermi Gamma-ray Space Telescope performed a ~6-day Target of Opportunity (ToO) observation of Nova Lupus 2016 (ATel #9538, #9539, CBET #4322) that commenced on September 28. Considering earlier all-sky survey Large Area Telescope (LAT) observations as well, preliminary analysis indicates gamma-ray emission at ~2 sigma was detected around 1 to 2 days after the optical peak on September 25th (pre-validated AAVSO visual lightcurve; ATel #9550, CBET #4322) when the optical spectra show opaque ejecta, similar to previous gamma-ray detected novae (Fermi-LAT collaboration, 2014 Science 345, 554; Cheung et al. 2016 ApJ 826, 142).

  3. Superhumps in the Rarely Outbursting SU UMa-Type Dwarf Nova, HO Delphini

    OpenAIRE

    Kato, T.; Nogami, D.; Moilanen, M. (Miika); 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 r...

  4. The electrification of Nova Scotia, 1884--1973: Technological modernization as a response to regional disparity

    Science.gov (United States)

    King, Lionel Bradley

    This dissertation investigates local attempts to use technology as a force for regional rehabilitation in the economically-depressed Maritime region of Canada. At the time of Confederation in 1867, the Maritime province of Nova Scotia was prosperous, progressive, and cultured. By the end of the 1910s, the province had entered a long period of economic and social decline. Recent historiography has shown that, far from passively accepting their fate, Nova Scotians and other Maritimers, actively resisted marginalization with political, cultural, or social action. The thesis expands upon that literature by exploring technology-based strategies of provincial rehabilitation using Thomas P. Hughes's systems perspective and David E. Nye's semiotic approach. In doing so, it applies methods from the social constructivist school of the history of technology to the larger concerns of Maritime Canadian historiography. In large part, the North American culture of technology determined the ways in which Nova Scotians applied technological solutions to provincial concerns. Technology has long been central to the Western idea of progress. As the "high technology" of the late nineteenth and early twentieth centuries, electricity reinforced that view: its ephemeral nature and silent efficiency led people to endow it with transformative, even mystical, powers. As a result, Nova Scotians, adopted a program of electrical modernization in the late 1910s as a remedy for regional disparity. The Nova Scotia government's first step was the creation of an Ontario-style hydroelectric commission designed to bring order to the province's fragmented and inefficient electrical network. Over the next few decades, the Nova Scotia Power Commission implemented rural electrification, home modernization, and regional system-building models that had already proven successful in Ontario and the United States. The system-building philosophies behind these programs were adapted to local conditions and

  5. An International Ultraviolet Explorer Archival Study of Dwarf Novae in Outburst

    Science.gov (United States)

    Hamilton, Ryan T.; Urban, Joel A.; Sion, Edward M.; Riedel, Adric R.; Voyer, Elysse N.; Marcy, John T.; Lakatos, Sarah L.

    2007-10-01

    We present a synthetic spectral analysis of nearly the entire far-ultraviolet International Ultraviolet Explorer (IUE) archive of spectra of dwarf novae in or near outburst. The study includes 46 systems of all dwarf nova subtypes, both above and below the period gap. The spectra were uniformly analyzed using synthetic spectral codes for optically thick accretion disks and stellar photospheres, along with the best available distance measurements or estimates. We present newly estimated accretion rates and discuss the implications of our study for disk accretion physics and CV evolution.

  6. Melostelis gen. nov., espécies novas e notas complementares sobre Anthidiini (Hymenoptera, Apidae

    Directory of Open Access Journals (Sweden)

    Danúncia Urban

    2011-06-01

    Full Text Available Melostelis gen. nov., espécies novas e notas complementares sobre Anthidiini (Hymenoptera, Apidae. Melostelis gen. nov. é proposto para um novo Anthidiini cleptoparasita. São descritas e ilustradas duas espécies novas: Melostelis amazonensis sp. nov. de Manaus, Amazonas e Larocanthidium chacoense sp. nov. de Porto Murtinho, Mato Grosso do Sul. São dados a conhecer os machos de Epanthidium bolivianum Urban, 1995 e Epanthidium araranguense Urban, 2006 e, registrados pela primeira vez no Brasil, na sub-região do chaco, Ketianthidium zanolae Urban, 2000 e Epanthidium bolivianum.

  7. Novas espécies de Esthlogena s. str. Thomson (Coleoptera, Cerambycidae, Lamiinae

    Directory of Open Access Journals (Sweden)

    Maria Helena M. Galileo

    2011-06-01

    Full Text Available Novas espécies de Esthlogena s. str. Thomson (Coleoptera, Cerambycidae, Lamiinae. Novas espécies de Pteropliini descritas: Esthlogena (E. nigrosuturalis do México e Panamá; E. (E. chicacaoensis e E. (E. amaliae da Guatemala; E. (E. dissimilis do Peru. Todas as espécies são ilustradas.New species of Esthlogena s. str. Thomson (Coleoptera, Cerambycidae, Lamiinae. New species described of Pteropliini: Esthlogena (E. nigrosuturalis from Mexico and Panama; E. (E. chicacaoensis and E. (E. amaliae from Guatemala; E. (E. dissimilis from Peru. All species are illustrated.

  8. Marketingový plán Nova Banka a.d. Banja Luka

    OpenAIRE

    Andžič, Srdjan

    2011-01-01

    The aim of this Master's thesis is to analyze marketing plan of Nova Bank A.D.Banja Luka from the year 2010. The theoretical part of the thesis describes the main parts of any marketing plan and creates the base for practical part of this thesis. Practical part starts with description od Nova Bank A.D. Banja Luka, it takes us deeper into issues. In the next step I'm creating the situation analysis of the bank, which helps me with analysing bank's marketing objectives and strategies. After tha...

  9. The 2010 early outburst spectrum of the recurrent nova U Scorpii

    CERN Document Server

    Kafka, Styliani

    2010-01-01

    Aims. We present optical spectra of the fast recurrent nova U Sco during its recent outburst, obtained within 24 hr of maximum light. Methods. We use medium resolution (R~4000) spectra taken with the with the MagE spectrograph on the Magellan (Clay) 6.5m telescope of the Las Campanas Observatories. Results. The spectrum is notable for its lack of a low ionization transient heavy element absorption system that is visible in the large majority of novae near maximum light. We suggest that this may be due to the dominance of inner Lagrangian L1 mass transfer and the absence of a circumbinary gas reservoir in this object

  10. Optical and Near-Infrared spectroscopy of Nova V1494 Aquilae 1999 #2

    CERN Document Server

    Kamath, U S; Ashok, N M; Mayya, Y D; Sahu, D K

    2005-01-01

    Optical and near-infrared spectroscopic observations of the fast nova V1494 Aquilae 1999 #2 covering various phases -- early decline, transition and nebular -- during the first eighteen months of its post-outburst evolution are presented in this paper. During this period, the nova evolved in the P_fe P_fe^o C_o spectral sequence. The transition from an optically thick wind to a polar blob - equatorial ring geometry is seen in the evolution of the spectral line profiles. There is evidence of density and temperature stratification in the ejecta. Physical conditions in the ejecta have been estimated based on our observations.

  11. High energy X-ray emission from recurrent novae in quiescence: T CrB

    CERN Document Server

    Luna, Gerardo J M; Mukai, Koji

    2007-01-01

    We present Suzaku X-ray observations of the recurrent nova T CrB in quiescence. T CrB is the first recurrent nova to be detected in the hard-X-ray band (E ~ 40.0 keV) during quiescence. The X-ray spectrum is consistent with cooling-flow emission emanating from an optically thin region in the boundary layer of an accretion disk around the white dwarf. The detection of strong stochastic flux variations in the light curve supports the interpretation of the hard X-ray emission as emanating from a boundary layer.

  12. An International Ultraviolet Explorer Archival Study of Dwarf Novae in Outburst

    CERN Document Server

    Hamilton, Ryan T; Sion, Edward M; Riedel, Adric R; Voyer, Elysse N; Marcy, John T; Lakatos, Sarah L

    2007-01-01

    We present a synthetic spectral analysis of nearly the entire far ultraviolet International Ultraviolet Explorer (IUE) archive of spectra of dwarf novae in or near outburst. The study includes 46 systems of all dwarf nova subtypes both above and below the period gap. The spectra were uniformly analyzed using synthetic spectral codes for optically thick accretion disks and stellar photospheres along with the best-available distance measurements or estimates. We present newly estimated accretion rates and discuss the implications of our study for disk accretion physics and CV evolution.

  13. EUVE All-Sky Survey Observations of the Dwarf Nova VW Hydri

    Science.gov (United States)

    Mauche, C. W.; Warren, J. K.; Vallerga, J. V.; Mukai, K.; Mattei, J. A.

    1993-05-01

    The dwarf nova VW Hyi was observed from 1992 November 1 to 18 and from November 20 to 23 by the Extreme Ultraviolet Explorer (EUVE) satellite during its all-sky survey. The total time on source was 22 kiloseconds. During the first part of the scan, VW Hyi was in quiescence following a superoutburst and was not detected by EUVE above background. However, the source went into a narrow outburst on November 13.8 U.T., peaked at V ~ 10 on November 14.8 U.T., started to fade on November 15.9 U.T., and returned to quiescence on November 17.8 U.T. In contrast, the source did not turn on in the EUV until November 15.0 U.T., did not peak until November 15.3 U.T., and had returned to quiescence by November 16.3 U.T. Accounting for the different sensitivities in the two wavebands, we conclude that the EUV outburst was delayed relative to the optical outburst by ~ 0.5 day and that the EUV outburst was narrower than the optical outburst by ~ 1 day. During the peak of the EUV outburst, the source was detected at the 3sigma level in the Lex/B (50--180 Angstroms ) scanner with a count rate of ~ 0.03 s(-1) and at the 4sigma level in the Al/Ti/C (160--240 Angstroms ) scanner with a count rate of ~ 0.09 s(-1) . That the Al/Ti/C count rate is significantly higher than the Lex/B count rate, whereas the effective area of the Al/Ti/C filter is smaller than that of the Lex/B filter, strongly indicates that the source was very soft when it was on. We use the count rates in these two filters to constrain the temperature and luminosity of the source of the shortest wavelength radiation in VW Hyi: the inner disk and the boundary layer between the disk and the surface of the white dwarf.

  14. Pelvic radiation - discharge

    Science.gov (United States)

    Radiation of the pelvis - discharge; Cancer treatment - pelvic radiation; Prostate cancer - pelvic radiation; Ovarian cancer - pelvic radiation; Cervical cancer - pelvic radiation; Uterine cancer - pelvic radiation; Rectal cancer - pelvic radiation

  15. Accretion-disc model spectra for dwarf-nova stars

    OpenAIRE

    Idan, Irit; Lasota, Jean-Pierre; Hameury, Jean-Marie; Shaviv, Giora

    2008-01-01

    Radiation from accretion discs in cataclysmic variable stars (CVs) provides fundamental information about the properties of these close binary systems and about the physics of accretion in general. The detailed diagnostics of accretion disc structure can be achieved by including in its description all the relevant heating and cooling physical mechanism, in particular the convective energy transport that, although dominant at temperatures less than about 10 000 K, is usually not taken into acc...

  16. Variação da razão entre fluxo sanguíneo e rotações da bomba centrífuga como ferramenta para monitorar o desempenho do oxigenador durante o suporte respiratório extracorpóreo

    Directory of Open Access Journals (Sweden)

    Marcelo Park

    2015-06-01

    Full Text Available RESUMO Objetivo: Analisar as correlações da taxa de fluxo sanguíneo e rotação da bomba com a pressão transmembrana e a transferência de CO2 e O2 durante o suporte respiratório extracorpóreo. Métodos: Cinco animais foram instrumentalizados e submetidos à oxigenação extracorpórea de membrana em um protocolo de cinco fases, as quais incluíam sepse abdominal e lesão pulmonar. Resultados: Este estudo demonstrou que as variações da taxa de fluxo sanguíneo e rotação da bomba dependem, de forma logarítmica positiva, do fluxo sanguíneo na membrana extracorpórea de oxigenação. As variações da taxa de fluxo sanguíneo e rotação da bomba têm associação negativa com a pressão transmembrana (R2 = 0,5 para o fluxo sanguíneo = 1.500mL/minuto e R2 = 0,4 para o fluxo sanguíneo = 3.500mL/minuto, ambos com p 6L/minuto, p = 0,006. A taxa de fluxo sanguíneo com a rotação da bomba não se associa às variações na transferência de O2 (R2 = 0,01 para o fluxo sanguíneo = 1.500mL/minuto, p = 0,19, e R2 = -0,01 ao fluxo sanguíneo = 3.500mL/minuto, p = 0,46. Conclusão: Neste modelo em animais, a variação da taxa de fluxo sanguíneo e rotação da bomba se associa negativamente com a pressão transmembrana e positivamente com a transferência de CO2. Conforme a situação clínica, uma diminuição na taxa do fluxo sanguíneo e rotação da bomba pode, na ausência de hipoxemia, indicar uma disfunção do pulmão artificial.

  17. Determination of natural radioactivity of groundwater and surface of Brumadinho and Nova Lima, Brazil; Determinacao da radioatividade natural de agua subterranea e superficial de Brumadinho e Nova Lima, Brasil

    Energy Technology Data Exchange (ETDEWEB)

    Faria, Ligia Santana de

    2013-07-01

    The municipalities of Brumadinho and Nova Lima are located in the metropolitan area of Belo Horizonte city. They are of ecological interest since they belong to an Environmental Protection Area, which is located on a very important deposit of iron ore. In addition of mineral wealth, the region has a geological characteristic that includes quartzitic conglomerates associated with uranium and significant potential underground water with hydrogeological characteristics very particular and complex, as the Quartzite Aquifer, which belongs to a geological formation called the 'Moeda Formation'. In the present work radiometric measurements were performed for 44 water samples. The samples were collected in four geographical points, three of them situated in Brumadinho (surface water) and one point situated in Nova Lima municipality (underground water). The period of sampling extended for a thirteen months period. Some of these locations was used as an alternative sampling point. Uranium and thorium concentrations of the samples were determined using an Inductively Coupled Plasma Mass Spectrometer. The content of gross alpha and gross beta activity, and the concentration of the radionuclides {sup 226}Ra, {sup 228}Ra e {sup 210}Pb were determinate by using Spectrometer Liquid Scintillation. In this case was necessary to calibrate the spectrometer using {sup 241}Am e {sup 90}Sr/{sup 90}Y standards. The resultants values were compared with those recommended by the World Health Organization, Ministry of Health and the National Council of the Environment. The maximum level of water natural radioactivity found was 0,275 ± 0,052 Bq.L{sup -1} for gross alpha radiation, 0,130 ± 0,046 Bq.L{sup -1} for {sup 226}Ra and 0,096 ± 0,005 Bq.L-1 for {sup 228}Ra. The levels of gross beta activity and {sup 210}Pb were below the detection limit. The maximum concentrations of uranium and thorium found were 0,068 μg.L{sup -1} and 0.027 μg.L{sup -1} respectively. (author)

  18. Atoms, Radiation, and Radiation Protection

    CERN Document Server

    Turner, James E

    2007-01-01

    Atoms, Radiation, and Radiation Protection offers professionals and advanced students a comprehensive coverage of the major concepts that underlie the origins and transport of ionizing radiation in matter. Understanding atomic structure and the physical mechanisms of radiation interactions is the foundation on which much of the current practice of radiological health protection is based. The work covers the detection and measurement of radiation and the statistical interpretation of the data. The procedures that are used to protect man and the environment from the potential harmful effects of

  19. Sustentabilidade de sistemas de rotação e sucessão de culturas em solos de várzea no Sul do Brasil Crop rotations sustainability and successions systems in tilled plain areas in Southern Brazil

    Directory of Open Access Journals (Sweden)

    Francisco de Jesus Vernetti Junior

    2009-09-01

    Full Text Available A avaliação quantitativa com diferentes tipos de indicadores é fundamental na determinação da sustentabilidade dos sistemas de rotação e sucessão de culturas. Este estudo teve como objetivo avaliar a sustentabilidade de algumas sucessões de culturas em solo de várzea, nos sistemas de plantio direto (PD e convencional (SC. O trabalho foi conduzido em Pelotas, Rio Grande do Sul (RS, em área experimental da Embrapa Clima Temperado. Os tratamentos foram constituídos por cinco anos de implantação de sistemas de rotação e sucessão de culturas de inverno e de primavera-verão, seguidos de dois anos de pousio e três anos da cultura do arroz irrigado. As culturas de primavera-verão foram o milho e a soja, além do arroz; enquanto que as de inverno foram gramíneas, leguminosas, consórcios, nabo forrageiro e campo natural. O delineamento experimental foi o de blocos ao acaso com parcelas subdivididas, com três repetições. As culturas de verão ocuparam as parcelas, enquanto as espécies de inverno foram alocadas nas subparcelas. Os parâmetros observados foram transformados em índices para padronizar as diversas variáveis, cada uma em relação àquela de melhor comportamento mensurado, e dispostos em quatro categorias de análise: (a indicadores agronômicos (matéria seca e rendimento de grãos; (b indicadores ambientais (fertilidade do solo; (c indicadores energéticos (produção e eficiência energética; d indicadores econômicos (valor bruto da produção e rentabilidade. Pela média harmônica obtida entre os índices dos indicadores, foram comparados os diferentes sistemas de rotação e sucessão de culturas, inferindo-se daí sua sustentabilidade e suas diferenças (Teste t P≤0,05. Concluiu-se que: (a todos os sistemas de rotação e sucessão de culturas dos quais o milho faz parte apresentam maior índice de sustentabilidade; (b os sistemas de rotação e sucessão de culturas S1 [gramínea x soja x arroz (PD] e S4

  20. Radiation Chemistry

    Science.gov (United States)

    Wojnárovits, L.

    Ionizing radiation causes chemical changes in the molecules of the interacting medium. The initial molecules change to new molecules, resulting in changes of the physical, chemical, and eventually biological properties of the material. For instance, water decomposes to its elements H2 and O2. In polymers, degradation and crosslinking take place. In biopolymers, e.g., DNS strand breaks and other alterations occur. Such changes are to be avoided in some cases (radiation protection), however, in other cases they are used for technological purposes (radiation processing). This chapter introduces radiation chemistry by discussing the sources of ionizing radiation (radionuclide sources, machine sources), absorption of radiation energy, techniques used in radiation chemistry research, and methods of absorbed energy (absorbed dose) measurements. Radiation chemistry of different classes of inorganic (water and aqueous solutions, inorganic solids, ionic liquids (ILs)) and organic substances (hydrocarbons, halogenated compounds, polymers, and biomolecules) is discussed in concise form together with theoretical and experimental backgrounds. An essential part of the chapter is the introduction of radiation processing technologies in the fields of polymer chemistry, food processing, and sterilization. The application of radiation chemistry to nuclear technology and to protection of environment (flue gas treatment, wastewater treatment) is also discussed.