中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Wind Roche lobe overflow as a way to make Type Ia supernovae from the widest symbiotic systems

文献类型:期刊论文

作者Ilkiewicz, Krystian1; Mikolajewska, Joanna1; Belczynski, Krzysztof1; Wiktorowicz, Grzegorz2,3; Karczmarek, Paulina4
刊名MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
出版日期2019-06-01
卷号485期号:4页码:5468-5473
关键词binaries: close binaries: symbiotic stars: evolution stars: individual: V407 Cyg supernovae: general
ISSN号0035-8711
DOI10.1093/mnras/stz760
英文摘要Symbiotic stars are interacting binaries with one of the longest known orbital periods. Because they can contain a massive white dwarf with a high accretion rate they are considered possible Type Ia supernova (SN Ia) progenitors. Among symbiotic binaries there are systems containing a Mira donor, which can have orbital periods of a few tens of years or more. This subclass of symbiotic stars has not usually been considered to provide promising SN Ia progenitors owing to their very large separation. We analyse the evolution of a well-studied symbiotic star with a Mira donor, V407 Cyg, and show that the standard evolution model predicts that the system will not become a SN Ia. However, with the addition of wind Roche lobe overflow as one of the mass-transfer modes, we predict that the white dwarf in V407 Cyg will reach the Chandrasekhar limit in 40-200 Myr.
WOS关键词WHITE-DWARF ; POPULATION SYNTHESIS ; GALACTIC POPULATION ; MASS-DISTRIBUTION ; RAY-EMISSION ; BLACK-HOLE ; V407 CYG ; PTF 11KX ; PROGENITORS ; EVOLUTION
资助项目Polish Ministry of Science and Higher Education Diamond Grant Programme[0136/DIA/2014/43] ; Foundation for Polish Science (FNP) within the START program ; Polish National Science Center (NCN)[OPUS 2017/27/B/ST9/01940] ; Polish National Science Center (NCN)[MAESTRO 2015/18/A/ST9/00746] ; NCN[Sonata Bis 2 2012/07/E/ST9/01360] ; NCN[OPUS 2015/19/B/ST9/01099] ; NCN[2015/19/B/ST9/03188] ; President's International Fellowship Initiative (PIFI) of the Chinese Academy of Sciences[2018PM0017] ; Strategic Priority Research Program of the Chinese Academy of Science 'Multi-waveband Gravitational Wave Universe'[XDB23040000]
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:000474880400074
出版者OXFORD UNIV PRESS
资助机构Polish Ministry of Science and Higher Education Diamond Grant Programme ; Polish Ministry of Science and Higher Education Diamond Grant Programme ; Foundation for Polish Science (FNP) within the START program ; Foundation for Polish Science (FNP) within the START program ; Polish National Science Center (NCN) ; Polish National Science Center (NCN) ; NCN ; NCN ; President's International Fellowship Initiative (PIFI) of the Chinese Academy of Sciences ; President's International Fellowship Initiative (PIFI) of the Chinese Academy of Sciences ; Strategic Priority Research Program of the Chinese Academy of Science 'Multi-waveband Gravitational Wave Universe' ; Strategic Priority Research Program of the Chinese Academy of Science 'Multi-waveband Gravitational Wave Universe' ; Polish Ministry of Science and Higher Education Diamond Grant Programme ; Polish Ministry of Science and Higher Education Diamond Grant Programme ; Foundation for Polish Science (FNP) within the START program ; Foundation for Polish Science (FNP) within the START program ; Polish National Science Center (NCN) ; Polish National Science Center (NCN) ; NCN ; NCN ; President's International Fellowship Initiative (PIFI) of the Chinese Academy of Sciences ; President's International Fellowship Initiative (PIFI) of the Chinese Academy of Sciences ; Strategic Priority Research Program of the Chinese Academy of Science 'Multi-waveband Gravitational Wave Universe' ; Strategic Priority Research Program of the Chinese Academy of Science 'Multi-waveband Gravitational Wave Universe' ; Polish Ministry of Science and Higher Education Diamond Grant Programme ; Polish Ministry of Science and Higher Education Diamond Grant Programme ; Foundation for Polish Science (FNP) within the START program ; Foundation for Polish Science (FNP) within the START program ; Polish National Science Center (NCN) ; Polish National Science Center (NCN) ; NCN ; NCN ; President's International Fellowship Initiative (PIFI) of the Chinese Academy of Sciences ; President's International Fellowship Initiative (PIFI) of the Chinese Academy of Sciences ; Strategic Priority Research Program of the Chinese Academy of Science 'Multi-waveband Gravitational Wave Universe' ; Strategic Priority Research Program of the Chinese Academy of Science 'Multi-waveband Gravitational Wave Universe' ; Polish Ministry of Science and Higher Education Diamond Grant Programme ; Polish Ministry of Science and Higher Education Diamond Grant Programme ; Foundation for Polish Science (FNP) within the START program ; Foundation for Polish Science (FNP) within the START program ; Polish National Science Center (NCN) ; Polish National Science Center (NCN) ; NCN ; NCN ; President's International Fellowship Initiative (PIFI) of the Chinese Academy of Sciences ; President's International Fellowship Initiative (PIFI) of the Chinese Academy of Sciences ; Strategic Priority Research Program of the Chinese Academy of Science 'Multi-waveband Gravitational Wave Universe' ; Strategic Priority Research Program of the Chinese Academy of Science 'Multi-waveband Gravitational Wave Universe'
源URL[http://ir.bao.ac.cn/handle/114a11/26948]  
专题中国科学院国家天文台
通讯作者Ilkiewicz, Krystian
作者单位1.Nicolaus Copernicus Astron Ctr, Bartycka 18, PL-00716 Warsaw, Poland
2.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
3.Univ Chinese Acad Sci, Sch Astron & Space Sci, Beijing 100012, Peoples R China
4.Univ Warsaw Observ, Al Ujazdowskie 4, PL-00478 Warsaw, Poland
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Ilkiewicz, Krystian,Mikolajewska, Joanna,Belczynski, Krzysztof,et al. Wind Roche lobe overflow as a way to make Type Ia supernovae from the widest symbiotic systems[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2019,485(4):5468-5473.
APA Ilkiewicz, Krystian,Mikolajewska, Joanna,Belczynski, Krzysztof,Wiktorowicz, Grzegorz,&Karczmarek, Paulina.(2019).Wind Roche lobe overflow as a way to make Type Ia supernovae from the widest symbiotic systems.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,485(4),5468-5473.
MLA Ilkiewicz, Krystian,et al."Wind Roche lobe overflow as a way to make Type Ia supernovae from the widest symbiotic systems".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 485.4(2019):5468-5473.

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