The diverse lives of progenitors of hydrogen-rich core-collapse supernovae: the role of binary interaction

doi:10.1051/0004-6361/201935854

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	The diverse lives of progenitors of hydrogen-rich core-collapse supernovae: the role of binary interaction
	Zapartas, Emmanouil 1,2,3; de Mink, Selma E.1,2,4; Justham, Stephen 1,2,5,6; Smith, Nathan 7; de Koter, Alex 1,2,8; Renzo, Mathieu 1,2; Arcavi, Iair 9; Farmer, Rob 1,2; Gotberg, Ylva 1,2,10; Toonen, Silvia 1,2,11,12
刊名	ASTRONOMY & ASTROPHYSICS
	2019-10-11
卷号	631 页码:19
关键词	supernovae: general binaries: close stars: massive stars: evolution
ISSN号	0004-6361
DOI	10.1051/0004-6361/201935854
英文摘要	Hydrogen-rich supernovae, known as Type II (SNe II), are the most common class of explosions observed following the collapse of the core of massive stars. We used analytical estimates and population synthesis simulations to assess the fraction of SNe II progenitors that are expected to have exchanged mass with a companion prior to explosion. We estimate that 1/3 to 1/2 of SN II progenitors have a history of mass exchange with a binary companion before exploding. The dominant binary channels leading to SN II progenitors involve the merger of binary stars. Mergers are expected to produce a diversity of SN II progenitor characteristics, depending on the evolutionary timing and properties of the merger. Alternatively, SN II progenitors from interacting binaries may have accreted mass from their companion, and subsequently been ejected from the binary system after their companion exploded. We show that the overall fraction of SN II progenitors that are predicted to have experienced binary interaction is robust against the main physical uncertainties in our models. However, the relative importance of different binary evolutionary channels is affected by changing physical assumptions. We further discuss ways in which binarity might contribute to the observed diversity of SNe II by considering potential observational signatures arising from each binary channel. For supernovae which have a substantial H-rich envelope at explosion (i.e., excluding Type IIb SNe), a surviving non-compact companion would typically indicate that the supernova progenitor star was in a wide, non-interacting binary. We argue that a significant fraction of even Type II-P SNe are expected to have gained mass from a companion prior to explosion.
资助项目	Netherlands Research School for Astronomy (NOVA) ; European Union's Horizon 2020 research and innovation program from the European Research Council (ERC) (Project BinCosmos)[715063] ; Netherlands Organisation for Scientific Research (NWO) as part of the Vidi research program BinWaves[639.042.728] ; NWO top grant[614.001.501]
WOS关键词	WOLF-RAYET STARS ; RED SUPERGIANT PROGENITOR ; MASSIVE CLOSE BINARIES ; STELLAR POPULATIONS ; IB SUPERNOVAE ; WHITE-DWARFS ; SN 1987A ; O-STARS ; EVOLUTION ; EXPLOSION
WOS研究方向	Astronomy & Astrophysics
语种	英语
出版者	EDP SCIENCES S A
WOS记录号	WOS:000515084100002
资助机构	Netherlands Research School for Astronomy (NOVA) ; Netherlands Research School for Astronomy (NOVA) ; European Union's Horizon 2020 research and innovation program from the European Research Council (ERC) (Project BinCosmos) ; European Union's Horizon 2020 research and innovation program from the European Research Council (ERC) (Project BinCosmos) ; Netherlands Organisation for Scientific Research (NWO) as part of the Vidi research program BinWaves ; Netherlands Organisation for Scientific Research (NWO) as part of the Vidi research program BinWaves ; NWO top grant ; NWO top grant ; Netherlands Research School for Astronomy (NOVA) ; Netherlands Research School for Astronomy (NOVA) ; European Union's Horizon 2020 research and innovation program from the European Research Council (ERC) (Project BinCosmos) ; European Union's Horizon 2020 research and innovation program from the European Research Council (ERC) (Project BinCosmos) ; Netherlands Organisation for Scientific Research (NWO) as part of the Vidi research program BinWaves ; Netherlands Organisation for Scientific Research (NWO) as part of the Vidi research program BinWaves ; NWO top grant ; NWO top grant ; Netherlands Research School for Astronomy (NOVA) ; Netherlands Research School for Astronomy (NOVA) ; European Union's Horizon 2020 research and innovation program from the European Research Council (ERC) (Project BinCosmos) ; European Union's Horizon 2020 research and innovation program from the European Research Council (ERC) (Project BinCosmos) ; Netherlands Organisation for Scientific Research (NWO) as part of the Vidi research program BinWaves ; Netherlands Organisation for Scientific Research (NWO) as part of the Vidi research program BinWaves ; NWO top grant ; NWO top grant ; Netherlands Research School for Astronomy (NOVA) ; Netherlands Research School for Astronomy (NOVA) ; European Union's Horizon 2020 research and innovation program from the European Research Council (ERC) (Project BinCosmos) ; European Union's Horizon 2020 research and innovation program from the European Research Council (ERC) (Project BinCosmos) ; Netherlands Organisation for Scientific Research (NWO) as part of the Vidi research program BinWaves ; Netherlands Organisation for Scientific Research (NWO) as part of the Vidi research program BinWaves ; NWO top grant ; NWO top grant
内容类型	期刊论文
源URL	[http://ir.bao.ac.cn/handle/114a11/54437]
专题	中国科学院国家天文台
通讯作者	Zapartas, Emmanouil
作者单位	1.Univ Amsterdam, Anton Pannekoek Inst Astron, NL-1090 GE Amsterdam, Netherlands 2.Univ Amsterdam, GRAPPA, NL-1090 GE Amsterdam, Netherlands 3.Univ Geneva, Geneva Observ, CH-1290 Sauverny, Switzerland 4.Harvard Smithsonian, Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA 5.Univ Chinese Acad Sci, Sch Astron & Space Sci, Beijing 100012, Peoples R China 6.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China 7.Univ Arizona, Steward Observ, 933 N Cherry Ave, Tucson, AZ 85721 USA 8.Katholieke Univ Leuven, Inst Astron, Celestijnenlaan 200 D, B-3001 Leuven, Belgium 9.Tel Aviv Univ, Sch Phys & Astron, IL-69978 Tel Aviv, Israel 10.Observ Carnegie Inst Sci, 813 Santa Barbara St, Pasadena, CA 91101 USA
推荐引用方式 GB/T 7714	Zapartas, Emmanouil,de Mink, Selma E.,Justham, Stephen,et al. The diverse lives of progenitors of hydrogen-rich core-collapse supernovae: the role of binary interaction[J]. ASTRONOMY & ASTROPHYSICS,2019,631:19.
APA	Zapartas, Emmanouil.,de Mink, Selma E..,Justham, Stephen.,Smith, Nathan.,de Koter, Alex.,...&Toonen, Silvia.(2019).The diverse lives of progenitors of hydrogen-rich core-collapse supernovae: the role of binary interaction.ASTRONOMY & ASTROPHYSICS,631,19.
MLA	Zapartas, Emmanouil,et al."The diverse lives of progenitors of hydrogen-rich core-collapse supernovae: the role of binary interaction".ASTRONOMY & ASTROPHYSICS 631(2019):19.