Stability and energetics of mass transfer in double white dwarfs | |
Han ZW(韩占文)1,2,3; Webbink, RF4; Han, ZW | |
发表期刊 | ASTRONOMY & ASTROPHYSICS |
1999-09 | |
卷号 | 349期号:1页码:L17-L20 |
产权排序 | 第1完成单位 |
收录类别 | SCI |
关键词 | Instabilities Stars : Binaries : Close Stars : White Dwarfs |
摘要 | The donor star in an interacting double white dwarf lies deep within the potential well of the accretor, a condition which both alters the minimum mass transfer rate needed to generate an Eddington luminosity, and limits the fraction of matter which can be driven from the binary in a super-Eddington wind. That mass loss itself alters the threshold condition for the onset of dynamical instability of the donor star. We show that, unless the mass of the accreting star is extremely near the Chandrasekhar limit, a significant fraction (exceeding 0.5 for accretors of mass < 1M(.)) must be retained, even when the; nominal accretion luminosity far exceeds the Eddington limit. In super-Eddington accretion, the accreted envelope almost certainly extends beyond the orbit of the donor, and will trigger white dwarf merger in a common envelope. |
语种 | 英语 |
学科领域 | Astronomy & Astrophysics |
文章类型 | Letter |
ISSN | 0004-6361 |
URL | 查看原文 |
WOS记录号 | WOS:000082912500005 |
WOS研究方向 | Astronomy & Astrophysics |
WOS类目 | Astronomy & Astrophysics |
关键词[WOS] | GRAVITATIONAL-RADIATION ; I SUPERNOVAE ; BINARIES ; STARS ; APPROXIMATIONS |
引用统计 | |
文献类型 | 期刊论文 |
条目标识符 | http://ir.ynao.ac.cn/handle/114a53/4389 |
专题 | 大样本恒星演化研究组 |
通讯作者 | Han, ZW |
作者单位 | 1.Yunnan Observatory, Academia Sinica, Kunming, 650011, P.R. China 2.National Astronomical Observatories, Chinese Academy of Sciences 3.Institute of Astronomy, Madingley Road, Cambridge, CB3 0HA, UK 4.Department of Astronomy, University of Illinois at Urbana-Champaign, 1002 West Green Street, Urbana, IL 61801, USA |
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 | Han ZW,Webbink, RF,Han, ZW. Stability and energetics of mass transfer in double white dwarfs[J]. ASTRONOMY & ASTROPHYSICS,1999,349(1):L17-L20. |
APA | Han ZW,Webbink, RF,&Han, ZW.(1999).Stability and energetics of mass transfer in double white dwarfs.ASTRONOMY & ASTROPHYSICS,349(1),L17-L20. |
MLA | Han ZW,et al."Stability and energetics of mass transfer in double white dwarfs".ASTRONOMY & ASTROPHYSICS 349.1(1999):L17-L20. |
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文件名称/大小 | 文献类型 | 版本类型 | 开放类型 | 使用许可 | ||
Stability and energe(107KB) | 期刊论文 | 作者接受稿 | 开放获取 | CC BY-NC-SA | 浏览 请求全文 |
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