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
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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.
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页码:537 / 543
页数:6
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