Binary Population Synthesis
Binary interactions lead to the formation of intriguing objects, such as compact binaries, supernovae, gamma ray bursts, X-ray binaries, pulsars, novae, cataclysmic variables, hot subdwarf stars, barium stars and blue stragglers. To study the evolution of binary populations and the consequent format...
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| Veröffentlicht in: | Research in astronomy and astrophysics 2020-10, Vol.20 (10), p.161 |
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| creator | Han, Zhan-Wen Ge, Hong-Wei Chen, Xue-Fei Chen, Hai-Liang |
| description | Binary interactions lead to the formation of intriguing objects, such as compact binaries, supernovae, gamma ray bursts, X-ray binaries, pulsars, novae, cataclysmic variables, hot subdwarf stars, barium stars and blue stragglers. To study the evolution of binary populations and the consequent formation of these objects, many methods have been developed over the years, for which a robust approach named binary population synthesis (BPS) warrants special attention. This approach has seen widespread application in many areas of astrophysics, including but not limited to analyses of the stellar content of galaxies, research on galactic chemical evolution and studies concerning star formation and cosmic re-ionization. In this review, we discuss the role of BPS, its general picture and the various components that comprise it. We pay special attention to the stability criteria for mass transfer in binaries, as this stability largely determines the fate of binary systems. We conclude with our perspectives regarding the future of this field. |
| doi_str_mv | 10.1088/1674-4527/20/10/161 |
| format | Article |
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Astron. Astrophys</addtitle><date>2020-10</date><risdate>2020</risdate><volume>20</volume><issue>10</issue><spage>161</spage><pages>161-</pages><issn>1674-4527</issn><abstract>Binary interactions lead to the formation of intriguing objects, such as compact binaries, supernovae, gamma ray bursts, X-ray binaries, pulsars, novae, cataclysmic variables, hot subdwarf stars, barium stars and blue stragglers. To study the evolution of binary populations and the consequent formation of these objects, many methods have been developed over the years, for which a robust approach named binary population synthesis (BPS) warrants special attention. This approach has seen widespread application in many areas of astrophysics, including but not limited to analyses of the stellar content of galaxies, research on galactic chemical evolution and studies concerning star formation and cosmic re-ionization. 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| source | IOP Publishing Journals; Alma/SFX Local Collection |
| subjects | Astrophysics Barium Binary stars Cataclysmic variables Chemical evolution Galactic evolution Galaxies galaxies: stellar content Gamma ray bursts Gamma rays Ionization Mass transfer methods: numerical Novae Pulsars Stability criteria Star & galaxy formation Star formation star: binaries (including multiple): close stars: evolution stars: statistics Stellar evolution Subdwarf stars Supernovae supernovae: general Synthesis X ray binaries X ray stars |
| title | Binary Population Synthesis |
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