Formation of hot subdwarf B stars with neutron star components | |
Wu Y(吴优)1,2,3; Chen XF(陈雪飞)1,2,4; Li ZW(李振威)1,2,3; Han ZW(韩占文)1,2,4 | |
刊名 | ASTRONOMY & ASTROPHYSICS |
2018-10-05 | |
卷号 | 618页码:12 |
关键词 | Binaries: General Stars: Formation Stars: Neutron Subdwarfs |
ISSN号 | 1432-0746 |
DOI | 10.1051/0004-6361/201832686 |
产权排序 | 第1完成单位 |
文献子类 | Article |
英文摘要 | Context. Binary population synthesis predicts the existence of subdwarf B stars (sdBs) with neutron star (NS) or black hole (BH) companions. Several works have been dedicated to finding such systems, but none has been confirmed yet. Theoretically, the formation of sdBs with white dwarf (WD) and main sequence (MS) companions has been well investigated, while those with NS or BH companions remain to be explored further. |
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 | Natural Science Foundation of China[11733008] ; Natural Science Foundation of China[11422324] ; Natural Science Foundation of China[11521303] ; Natural Science Foundation of Yunnan province[2017HC018] ; Natural Science Foundation of Yunnan province[2013HA005] |
WOS关键词 | White-dwarf Companions ; Electron-capture Supernovae ; Initial Mass Function ; O-type Subdwarf ; Millisecond Pulsars ; Hd 49798 ; Population Synthesis ; Driving Mechanism ; Radio Pulsars ; Kpd 1930+2752 |
WOS研究方向 | Astronomy & Astrophysics |
语种 | 英语 |
出版者 | EDP SCIENCES S A |
WOS记录号 | WOS:000446426500002 |
资助机构 | Natural Science Foundation of China[11733008, 11422324, 11521303] ; Natural Science Foundation of Yunnan province[2017HC018, 2013HA005] |
内容类型 | 期刊论文 |
源URL | [http://ir.ynao.ac.cn/handle/114a53/18025] |
专题 | 云南天文台_大样本恒星演化研究组 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 | Wu Y(吴优) |
作者单位 | 1.Yunnan Observatories, Chinese Academy of Sciences, Kunming 650216, PR China 2.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming 650216, PR China 3.University of the Chinese Academy of Science, Beijing 100049, PR China 4.Center for Astronomical Mega-Science, Chinese Academy of Sciences, 20A Datun Road, Chaoyang District, Beijing 100012, PR China |
推荐引用方式 GB/T 7714 | Wu Y,Chen XF,Li ZW,et al. Formation of hot subdwarf B stars with neutron star components[J]. ASTRONOMY & ASTROPHYSICS,2018,618:12. |
APA | Wu Y,Chen XF,Li ZW,&Han ZW.(2018).Formation of hot subdwarf B stars with neutron star components.ASTRONOMY & ASTROPHYSICS,618,12. |
MLA | Wu Y,et al."Formation of hot subdwarf B stars with neutron star components".ASTRONOMY & ASTROPHYSICS 618(2018):12. |
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