The possible formation of massive tori in white-dwarf binary systems

被引:0
作者
D. P. Savokhin
E. I. Staritsyn
机构
[1] Ural State University,Astronomical Observatory
来源
Astronomy Reports | 2002年 / 46卷
关键词
Binary System; Total Masse; Mass Exchange; Massive Component; Massive Torus;
D O I
暂无
中图分类号
学科分类号
摘要
Mass exchange in white-dwarf binary systems with mass ratios 0.35–0.55 and total masses exceeding the Chandrasekhar limit could lead to the disruption of the less massive component of the system and the formation of a torus around the more massive component.
引用
收藏
页码:481 / 488
页数:7
相关论文
共 73 条
[1]  
Tutukov A. V.(1979)undefined Acta Astron. 29 665-undefined
[2]  
Yungelson L. R.(1984)undefined Astrophys. J. 282 615-undefined
[3]  
Iben I.(2001)undefined Astron. Astrophys. 365 491-undefined
[4]  
Tutukov A. V.(2000)undefined Astron. Astrophys. 360 1011-undefined
[5]  
Nelemans G.(1995)undefined Mon. Not. R. Astron. Soc. 275 828-undefined
[6]  
Yungelson L. R.(2000)undefined Mon. Not. R. Astron. Soc. 314 334-undefined
[7]  
Portegis Zwart S. F.(1995)undefined Mon. Not. R. Astron. Soc. 275 L1-undefined
[8]  
Verbunt F.(1997)undefined Mon. Not. R. Astron. Soc. 288 538-undefined
[9]  
Nelemans G.(1997)undefined Astrophys. J. 475 291-undefined
[10]  
Verbunt F.(2000)undefined Mon. Not. R. Astron. Soc. 317 L41-undefined