Superhumps in binary systems and their connection to precessional spiral density waves

被引：0
|
作者：
P. V. Kaĭgorodov
D. V. Bisikalo
O. A. Kuznetsov
A. A. Boyarchuk
机构：
[1] Institute of Astronomy,
[2] Keldysh Institute of Applied Mathematics,undefined
来源：
Astronomy Reports | 2006年 / 50卷
关键词：
97.80.G;
D O I：
暂无
中图分类号：
学科分类号：
摘要：
We consider a mechanism for the formation of superhumps in the TV Col system, based on the possible existence of a precessional spiral wave in the accretion disk of the system. This mechanism can act in binaries with arbitrary component-mass ratios, and our precessional spiral wave model can be applied to explain observed superhumps of all types.
引用
收藏
页码：537 / 543
页数：6
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