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

被引：9
|
作者：
Kaigorodov, P. V. [1 ]
Bisikalo, D. V.
Kuznetsov, O. A.
Boyarchuk, A. A.
机构：
[1] Russian Acad Sci, Inst Astron, Moscow, Russia
[2] MV Keldysh Appl Math Inst, Moscow 125047, Russia
来源：
ASTRONOMY REPORTS | 2006年 / 50卷 / 07期
基金：
俄罗斯基础研究基金会;
关键词：
D O I：
10.1134/S1063772906070031
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
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：7
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