The spin of the second-born black hole in coalescing binary black holes | |
Qin, Y.1; Fragos, T.1,2; Meynet, G.1; Andrews, J.3,4; Sorensen, M.1; Song, H. F.1,5,6 | |
刊名 | ASTRONOMY & ASTROPHYSICS |
2018-08-10 | |
卷号 | 616 |
关键词 | Binaries: Close Stars: Black Holes Stars: Evolution Sun: Rotation Gamma-ray Burst: General Stars: Wolf-rayet |
ISSN号 | 1432-0746 |
DOI | 10.1051/0004-6361/201832839 |
文献子类 | Article |
英文摘要 | Context. Various binary black hole formation channels have been proposed since the first gravitational event GW150914 was discovered by the Advanced Laser Interferometer Gravitational-Wave Observatory (AdLIGO). The immediate progenitor of the binary black hole is a close binary system composed of a black hole and a helium star, which can be the outcome of the classical isolated binary evolution through the common envelope, or alternatively of the massive close evolution through chemically homogeneous channel. |
学科主题 | 天文学 |
URL标识 | 查看原文 |
出版地 | 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A, FRANCE |
资助项目 | China Scholarship Council (CSC) ; Swiss National Science Foundation[200020-172505] ; Swiss National Science Foundation[PZ00P2_148123] ; European Unions Horizon 2020 research and innovation program under the Marie Sklodowska-Curie RISE action[691164] ; DNRF (Niels Bohr Professorship Program) ; Carlsberg Foundation ; VILLUM FONDEN[16599] ; European Research Council under the European Union's Seventh Framework Programme/ERC Grant[617001] |
WOS关键词 | Gamma-ray Bursts ; Rotating Massive Stars ; Differential Rotation ; Gravitational-waves ; Tidal-evolution ; Magnetic-fields ; Main-sequence ; Neutron-star ; Stellar ; Progenitors |
WOS研究方向 | Astronomy & Astrophysics |
语种 | 英语 |
出版者 | EDP SCIENCES S A |
WOS记录号 | WOS:000441203300001 |
资助机构 | China Scholarship Council (CSC) ; Swiss National Science Foundation[200020-172505, PZ00P2_148123] ; European Unions Horizon 2020 research and innovation program under the Marie Sklodowska-Curie RISE action[691164] ; DNRF (Niels Bohr Professorship Program) ; Carlsberg Foundation ; VILLUM FONDEN[16599] ; European Research Council under the European Union's Seventh Framework Programme/ERC Grant[617001] |
内容类型 | 期刊论文 |
源URL | [http://ir.ynao.ac.cn/handle/114a53/17389] |
专题 | 云南天文台_中国科学院天体结构与演化重点实验室 |
通讯作者 | Qin, Y. |
作者单位 | 1.Geneva Observatory, University of Geneva, 1290 Sauverny, Switzerland 2.DARK, Niels Bohr Institute, University of Copenhagen, 2100 Copenhagen, Denmark 3.Foundation for Research and Technology – Hellas, IESL, Voutes, 71110 Heraklion, Greece 4.Physics Department & Institute of Theoretical & Computational Physics, University of Crete, 71003 Heraklion, Crete, Greece 5.College of Physics, Guizhou University, Guiyang City, Guizhou Province, 550025, PR China 6.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming 650011, PR China |
推荐引用方式 GB/T 7714 | Qin, Y.,Fragos, T.,Meynet, G.,et al. The spin of the second-born black hole in coalescing binary black holes[J]. ASTRONOMY & ASTROPHYSICS,2018,616. |
APA | Qin, Y.,Fragos, T.,Meynet, G.,Andrews, J.,Sorensen, M.,&Song, H. F..(2018).The spin of the second-born black hole in coalescing binary black holes.ASTRONOMY & ASTROPHYSICS,616. |
MLA | Qin, Y.,et al."The spin of the second-born black hole in coalescing binary black holes".ASTRONOMY & ASTROPHYSICS 616(2018). |
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