Wave-warp resonant interactions in relativistic disks and kHz QPOs

被引:27
作者
Kato, S [1 ]
机构
[1] Nara Sangyo Univ, Dept Informat, Nara 6368503, Japan
关键词
accretion; accretion disks; kHz quasi-periodic oscillations; relativity; warps; X-rays : stars;
D O I
10.1093/pasj/56.3.559
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Non-linear resonant interactions between disk oscillations and relativistic disks are examined under the assumption that the disks are deformed by a warp. There are three types of resonances: horizontal and vertical resonances of g-mode oscillations, and horizontal resonances of p-mode oscillations. In the limit of long-wavelength oscillations, the resonances occur at 3r(g), 3.62r(g), 4r(g), and 6.46r(g), depending on the types of resonances and the wave modes. The frequencies of the resonant oscillations at these points also depend on the modes of oscillations. There are sets of resonant oscillations whose frequency ratio is close to 2 : 3. The frequencies of the resonant oscillations can change as a wave packet propagates in the radial direction.
引用
收藏
页码:559 / 567
页数:9
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