Companion stars of type Ia supernovae and hypervelocity stars | |
Wang B(王博)1,2; Han ZW(韩占文)1; Wang, B (reprint author), Chinese Acad Sci, Natl Astron Observ, Yunnan Observ, Kunming 650011, Peoples R China. | |
发表期刊 | ASTRONOMY & ASTROPHYSICS |
2009-12 | |
卷号 | 508期号:2页码:L27-L30 |
DOI | 10.1051/0004-6361/200913326 |
产权排序 | 第1完成单位 |
收录类别 | SCI ; EI |
关键词 | Binaries: General Supernovae: General Stars: Evolution White Dwards |
摘要 | Context. Recent investigations of the white dwarf (WD) + He star channel of Type Ia supernovae (SNe Ia) imply that this channel can produce SNe Ia with short delay times. The companion stars in this channel would survive and potentially be identifiable. Aims. In this Letter, we study the properties of the companion stars of this channel at the moment of SN explosion, which can be verified by future observations. Methods. According to SN Ia production regions of the WD + He star channel and three formation channels of WD + He star systems, we performed a detailed binary population synthesis study to obtain the properties of the surviving companions. Results. We obtained the distributions of many properties of the companion stars of this channel at the moment of SN explosion. We find that the surviving companion stars have a high spatial velocity (> 400 km s(-1)) after SN explosion, which could be an alternative origin for hypervelocity stars (HVSs), especially for HVSs such as US 708. |
项目资助者 | National Natural Science Foundation of China [10821061] ; National Basic Research Program of China [2007CB815406] ; Yunnan Natural Science Foundation [08YJ041001] |
语种 | 英语 |
学科领域 | Astronomy & Astrophysics |
文章类型 | Article |
ISSN | 0004-6361 |
URL | 查看原文 |
归档日期 | 2009-12-14 |
WOS记录号 | WOS:000273296700002 |
WOS研究方向 | Astronomy & Astrophysics |
WOS类目 | Astronomy & Astrophysics |
关键词[WOS] | SINGLE-DEGENERATE CHANNEL ; SUBDWARF-B-STARS ; WHITE-DWARF ; BLACK-HOLE ; SYMBIOTIC CHANNEL ; BINARY-SYSTEMS ; DELAY TIMES ; PROGENITORS ; EVOLUTION ; MASS |
引用统计 | |
文献类型 | 期刊论文 |
条目标识符 | http://ir.ynao.ac.cn/handle/114a53/4464 |
专题 | 大样本恒星演化研究组 |
通讯作者 | Wang, B (reprint author), Chinese Acad Sci, Natl Astron Observ, Yunnan Observ, Kunming 650011, Peoples R China. |
作者单位 | 1.National Astronomical Observatories/Yunnan Observatory, the Chinese Academy of Sciences, Kunming 650011, PR China 2.Graduate University of the Chinese Academy of Sciences, Beijing 100049, PR China |
第一作者单位 | 中国科学院云南天文台 |
推荐引用方式 GB/T 7714 | Wang B,Han ZW,Wang, B . Companion stars of type Ia supernovae and hypervelocity stars[J]. ASTRONOMY & ASTROPHYSICS,2009,508(2):L27-L30. |
APA | Wang B,Han ZW,&Wang, B .(2009).Companion stars of type Ia supernovae and hypervelocity stars.ASTRONOMY & ASTROPHYSICS,508(2),L27-L30. |
MLA | Wang B,et al."Companion stars of type Ia supernovae and hypervelocity stars".ASTRONOMY & ASTROPHYSICS 508.2(2009):L27-L30. |
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