Academic literature on the topic 'Binary stellar evolution'
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Journal articles on the topic "Binary stellar evolution"
Batten, A. H. "Stellar evolution in binary systems." Reports on Progress in Physics 58, no. 8 (August 1, 1995): 885–928. http://dx.doi.org/10.1088/0034-4885/58/8/002.
Full textChen, Xuefei, and Zhanwen Han. "Primordial binary evolution and blue stragglers." Proceedings of the International Astronomical Union 5, S266 (August 2009): 333–38. http://dx.doi.org/10.1017/s1743921309991220.
Full textSiess, L., R. G. Izzard, P. J. Davis, and R. Deschamps. "BINSTAR: a new binary stellar evolution code." Astronomy & Astrophysics 550 (February 2013): A100. http://dx.doi.org/10.1051/0004-6361/201220327.
Full textMcMillan, Stephen L. W. "Star Cluster Simulations Including Stellar Evolution." Symposium - International Astronomical Union 208 (2003): 131–44. http://dx.doi.org/10.1017/s0074180900207092.
Full textHatfull, Roger W. M., Natalia Ivanova, and James C. Lombardi. "Simulating a stellar contact binary merger – I. Stellar models." Monthly Notices of the Royal Astronomical Society 507, no. 1 (July 26, 2021): 385–97. http://dx.doi.org/10.1093/mnras/stab2140.
Full textCzesla, S., S. Terzenbach, R. Wichmann, and J. H. M. M. Schmitt. "Spot evolution in the eclipsing binary CoRoT 105895502." Astronomy & Astrophysics 623 (March 2019): A107. http://dx.doi.org/10.1051/0004-6361/201834516.
Full textEggleton, Peter P. "Combining Stellar Evolution and Stellar Dynamics." Symposium - International Astronomical Union 174 (1996): 213–22. http://dx.doi.org/10.1017/s0074180900001558.
Full textPetrovic, Jelena. "The evolution of massive binary systems." Serbian Astronomical Journal, no. 201 (2020): 1–13. http://dx.doi.org/10.2298/saj2001001p.
Full textStairs, I. H. "Pulsars in Binary Systems: Probing Binary Stellar Evolution and General Relativity." Science 304, no. 5670 (April 23, 2004): 547–52. http://dx.doi.org/10.1126/science.1096986.
Full textEldridge, J. J. "The things binaries do …" Astronomy & Geophysics 61, no. 2 (April 1, 2020): 2.24–2.29. http://dx.doi.org/10.1093/astrogeo/ataa029.
Full textDissertations / Theses on the topic "Binary stellar evolution"
Pols, Onno Rudolf. "On the evolution of massive close binary stars in stellar populations." Amsterdam : Amsterdam : Sterrenkundig Instituut 'Anton Pannekoek' ; Universiteit van Amsterdam [Host], 1993. http://dare.uva.nl/document/91990.
Full textBarrett, James William. "Topics in astrostatistics : stellar binary evolution, gravitational-wave source modelling and stochastic processes." Thesis, University of Birmingham, 2018. http://etheses.bham.ac.uk//id/eprint/8203/.
Full textSaffer, R. A., and J. Liebert. "Search for Close Binary Evolved Stars." Steward Observatory, The University of Arizona (Tucson, Arizona), 1988. http://hdl.handle.net/10150/623897.
Full textOhlmann, Sebastian Thomas [Verfasser], and Friedrich [Akademischer Betreuer] Röpke. "Hydrodynamics of the Common Envelope Phase in Binary Stellar Evolution / Sebastian Thomas Ohlmann ; Betreuer: Friedrich Röpke." Heidelberg : Universitätsbibliothek Heidelberg, 2016. http://d-nb.info/1180615891/34.
Full textOhlmann, Sebastian T. [Verfasser], and Friedrich [Akademischer Betreuer] Röpke. "Hydrodynamics of the Common Envelope Phase in Binary Stellar Evolution / Sebastian Thomas Ohlmann ; Betreuer: Friedrich Röpke." Heidelberg : Universitätsbibliothek Heidelberg, 2016. http://nbn-resolving.de/urn:nbn:de:bsz:16-heidok-215131.
Full textMoran, Chris. "Using observations of detached double degenerate binaries to test theories of stellar evolution in close binary systems." Thesis, University of Southampton, 1999. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.310751.
Full textDouchin, Dimitri. "Estimation de la fraction binaire de nébuleuses planétaires." Thesis, Montpellier 2, 2014. http://www.theses.fr/2014MON20069/document.
Full textPlanetary nebulae (PNe) are the products of the evolution of intermediate mass stars that have expanded spherically at the end of their lives. Observationally, it has been estimated that 80% of them have non-spherical shapes. Such a high fraction is puzzling and has occupied the PN community for more than 30 years. One scenario that would allow to justify the observed shapes is that a comparable fraction of the progenitors of central stars of PN (CSPN) are not single, but possess a companion. The shape of the nebulae would then be the result of an interaction with this companion. The high fraction of non-spherical PNe would thus imply a high fraction of binary CSPN, making binarity a preferred channel for PN formation. After presenting the current state of knowledge regarding PN formation and shaping and reviewing the diverse efforts to find binaries in PNe, I present my work to detect a near-infrared excess that would be the signature of the presence of cool companions. The first part of the project consists in the analysis of data and photometry acquired and conducted by myself. The second part details an attempt to make use of archived datasets: the Sloan Digital Sky Survey Data Release 7 optical survey and the extended database assembled by Frew (2008). I also present results from a radial velocity analysis of VLT/UVES spectra for 14 objects aiming to the detection of spectroscopic companions. Finally I give details of the analysis of optical photometry data from our observations associated to the detection of companions around CSPN using the photometric variability technique. The main result of this thesis is from the near-infrared excess studies which I combine with previously-published data. I conclude that the if the detected red and NIR flux excess is indicative of a stellar companion then the binary fraction is larger than what we may expect based on the main-sequence progenitor population binary fraction and therefore conclude that binarity is a preferential channel for the formation of PN. I finish by underlining the need for a sample size of ∼ 150 objects to decrease the uncertainty on the PN population binary fraction and increase the statistical significance of this result
Deschamps, Romain. "Evolution of low and intermediate mass stars in binary systems: a new look at Algol systems." Doctoral thesis, Universite Libre de Bruxelles, 2015. http://hdl.handle.net/2013/ULB-DIPOT:oai:dipot.ulb.ac.be:2013/209077.
Full textstill rather poorly understood. We know that they are composed by a generally B-A main sequence
star and a lighter but more evolved companion star. This paradox is explained by the transfer of mass
between the two stars, but new problems arose. In particular, I studied the mass-transfer driven spin-
up of the accreting star that drives the star to critical rotation and the puzzling, indirectly observed, non-conservative evolution.
Doctorat en Sciences
info:eu-repo/semantics/nonPublished
Santos, Leonardo Augusto Gonçalves dos. "The rotational evolution of Sun-like stars and the influence of low-mass binary companions." Universidade de São Paulo, 2017. http://www.teses.usp.br/teses/disponiveis/14/14131/tde-22052018-174015/.
Full textO programa The Solar Twin Planet Search é um esforço sem precedentes na procura de planetas extra-solares em mais de 70 estrelas extremamente similares ao Sol. Ao longo desse programa, centenas de espectros ópticos de alta qualidade foram obtidos com o espectrógrafo HARPS, que está instalado no telescópio de 3,6 m do Observatório de La Silla. Além da busca de exoplanetas, estes dados são úteis para estudar as propriedades físicas de estrelas como o Sol. Estamos interessados em verificar se o Sol possui uma rotação regular para sua idade quando comparado com estrelas estritamente similares a ele, como que a rotação de gêmeas solares evolui com o tempo e se a rotação dessas estrelas é influenciada pela presença de companheiras estelares. Conclusões anteriores na regularidade da rotação solar são conflitantes, e esta é a primeira vez que uma amostra grande de gêmeas solares com dados espectroscópicos de alta qualidade é usada para esclarecer essa questão. Nossos resultados sugerem que o Sol de fato rota regularmente para sua idade, o que favorece o uso da rotação solar para calibrar a girocronologia -- a estimativa de idades estelares a partir de sua rotação. No entanto, tais resultados também implicam em um processo de evolução rotacional que satura depois da idade solar, constituindo um desvio da amplamente usada relação de Skumanich e apresentando um desafio para a girocronologia. Nós identificamos 18 sistemas binários na amostra de gêmeas solares, das quais apenas três mostram rotações elevadas para suas idades. Os parâmetros orbitais das binárias foram estimados a partir da variação de suas velocidades radiais, e os resultados mostram que suas companheiras espectroscópicas possuem períodos orbitais variando de alguns poucos até muitos anos. Concluimos que a presença de companheiras do tipo anãs vermelhas ou marrons em períodos orbitais moderados não influenciam a evolução rotacional desses sistemas. As peculiaridades de HIP 19911, HIP 67620 e HIP 103983 podem ser completamente explicadas por contaminação espectral de suas companheiras.
Karakas, Amanda I. (Amanda Irene) 1974. "Asymptotic giant branch stars : their influence on binary systems and the interstellar medium." Monash University, School of Mathematical Sciences, 2003. http://arrow.monash.edu.au/hdl/1959.1/5570.
Full textBooks on the topic "Binary stellar evolution"
Boffin, Henri M. J., and Giacomo Beccari. Impact of Binary Stars on Stellar Evolution. Cambridge University Press, 2019.
Find full textBoffin, Henri M. J., and Giacomo Beccari. Impact of Binary Stars on Stellar Evolution. University of Cambridge ESOL Examinations, 2019.
Find full textBoffin, Henri M. J., and Giacomo Beccari. Impact of Binary Stars on Stellar Evolution. Cambridge University Press, 2019.
Find full textBeccari, Giacomo, and Henri M. J. Boffin, eds. The Impact of Binary Stars on Stellar Evolution. Cambridge University Press, 2019. http://dx.doi.org/10.1017/9781108553070.
Full textOn the evolution, numbers, and characteristics of close-binary supersoft sources. [Washington, DC: National Aeronautics and Space Administration, 1996.
Find full textKopal, Zdenek. Binary and Multiple Stars as Tracers of Stellar Evolution: "Proceedings of the 69th Colloquium of the International Astronomical Union, Held in ... Ingramcontent, 2011.
Find full textTidal evolution and oscillations in binary stars: Third Granada workshop on stellar structure : proceedings of a workshop held in Granada, Spain, 26-28 May 2004. San Francisco, CA: Astronomical Society of the Pacific, 2006.
Find full textAntonio, Claret, Giménez Alvaro, and Zahn Jean-Paul, eds. Tidal evolution and oscillations in binary stars: Third Granada workshop on stellar structure : proceedings of a workshop held in Granada, Spain, 26-28 May 2004. San Francisco, Calif: Astronomical Society of the Pacific, 2005.
Find full textUnited States. National Aeronautics and Space Administration., ed. Collaborative observations of HDE 332077. [Washington, DC: National Aeronautics and Space Administration, 1995.
Find full textClaret, Antonio. Tidal Evolution and Oscillations in Binary Stars: Third Granada Workshop on Stellar Structure: Proceedings of a Workshop Held in Granada, Spain, 26-28 (Astronomical Society of the Pacific Conference). Astronomical Society of the Pacific, 2005.
Find full textBook chapters on the topic "Binary stellar evolution"
Benacquista, Matthew. "Stellar Evolution Equations." In An Introduction to the Evolution of Single and Binary Stars, 47–61. New York, NY: Springer New York, 2012. http://dx.doi.org/10.1007/978-1-4419-9991-7_4.
Full textDe Loore, C. W. H., and C. Doom. "Stellar Convection." In Structure and Evolution of Single and Binary Stars, 119–36. Dordrecht: Springer Netherlands, 1992. http://dx.doi.org/10.1007/978-94-011-2502-4_7.
Full textBenvenuto, Omar G., and Melina C. Bersten. "Close Binary Stellar Evolution and Supernovae." In Handbook of Supernovae, 1–22. Cham: Springer International Publishing, 2017. http://dx.doi.org/10.1007/978-3-319-20794-0_124-1.
Full textBenvenuto, Omar G., and Melina C. Bersten. "Close Binary Stellar Evolution and Supernovae." In Handbook of Supernovae, 649–70. Cham: Springer International Publishing, 2017. http://dx.doi.org/10.1007/978-3-319-21846-5_124.
Full textBenacquista, Matthew. "Stellar Birth." In An Introduction to the Evolution of Single and Binary Stars, 133–46. New York, NY: Springer New York, 2012. http://dx.doi.org/10.1007/978-1-4419-9991-7_10.
Full textFrankowski, Adam. "AGB Evolution in Binary Systems." In Post-AGB Objects as a Phase of Stellar Evolution, 173–80. Dordrecht: Springer Netherlands, 2001. http://dx.doi.org/10.1007/978-94-015-9688-6_27.
Full textEggleton, Peter P., and Ludmila G. Kiseleva. "Stellar and Dynamical Evolution within Triple Stars." In Evolutionary Processes in Binary Stars, 345–64. Dordrecht: Springer Netherlands, 1996. http://dx.doi.org/10.1007/978-94-009-1673-9_17.
Full textBenacquista, Matthew. "Simple Stellar Models." In An Introduction to the Evolution of Single and Binary Stars, 107–18. New York, NY: Springer New York, 2012. http://dx.doi.org/10.1007/978-1-4419-9991-7_8.
Full textPringle, J. E. "Binary Star Formation." In The Physics of Star Formation and Early Stellar Evolution, 437–48. Dordrecht: Springer Netherlands, 1991. http://dx.doi.org/10.1007/978-94-011-3642-6_12.
Full textDe Loore, C. W. H., and C. Doom. "The Equations of Stellar Structure." In Structure and Evolution of Single and Binary Stars, 22–35. Dordrecht: Springer Netherlands, 1992. http://dx.doi.org/10.1007/978-94-011-2502-4_2.
Full textConference papers on the topic "Binary stellar evolution"
Lister, T. A., and Eric Stempels. "Long term evolution of surface features on the unusual close binary V361 Lyr." In COOL STARS, STELLAR SYSTEMS AND THE SUN: Proceedings of the 15th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun. AIP, 2009. http://dx.doi.org/10.1063/1.3099207.
Full textMarov, M. Ya, and I. I. Shevchenko. "Planets — a modern view." In ASTRONOMY AT THE EPOCH OF MULTIMESSENGER STUDIES. Proceedings of the VAK-2021 conference, Aug 23–28, 2021. Crossref, 2022. http://dx.doi.org/10.51194/vak2021.2022.1.1.005.
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