Spiral shocks in the accretion disk of the dwarf nova U Geminorum

被引:0
|
作者
Neustroev, VV
Borisov, NV
机构
[1] Udmurt State Univ, Dept Astron & Mech, Izhevsk 426034, Russia
[2] Special Astrophys Observ, Karachaevo Cherkesia 357147, Russia
来源
ASTRONOMY & ASTROPHYSICS | 1998年 / 336卷 / 03期
关键词
accretion; accretion disks; line : profiles; line : formation; novae; cataclysmic variables; stars : individual : U Gem;
D O I
暂无
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present a study of the observable spectral manifestations associated with spiral shocks within quiescent accretion disks and compare them with observations of the dwarf nova U Geminorum. Our results indicate that the orbital behaviour of the hydrogen emission line profile in the spectrum of U Gem can be reproduced via a simple model of the accretion disk with two symmetrically located spiral shocks with the spiral angle theta about 60 degrees. This provides for the first time convincing evidence for the existence of spiral shocks in the accretion disk of a cataclysmic variable in quiescence.
引用
收藏
页码:L73 / L76
页数:4
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