机构:
Univ Sydney, Sch Phys, Res Ctr Theoret Astrophys, Sydney, NSW 2006, AustraliaUniv Sydney, Sch Phys, Res Ctr Theoret Astrophys, Sydney, NSW 2006, Australia
Wu, KW
[1
]
机构:
[1] Univ Sydney, Sch Phys, Res Ctr Theoret Astrophys, Sydney, NSW 2006, Australia
来源:
ACCRETION PHENOMENA AND RELATED OUTFLOWS: IAU COLLOQUIUM 163
|
1997年
/
121卷
关键词:
D O I:
暂无
中图分类号:
P1 [天文学];
学科分类号:
0704 ;
摘要:
The mass transfer process in low mass close binaries is reviewed. The driving mechanisms and the stability properties are discussed by means of general, simple formulations. A model in terms of mass transfer instabilities is suggested to explain the outbursts of GRO J1655-40 in 1994.