A resonance model of quasi-periodic oscillations of low-mass X-ray binaries

被引：11
|
作者：
Kato, S [1 ]
机构：
[1] Nara Sangyo Univ, Dept Informat, Nara 6368503, Japan
来源：
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN | 2005年 / 57卷 / 03期
关键词：
accretion; accrection disks; hectohertz QPOs; horizontal branch QPOs; kHz QPOs; relativity; resonance; warp; X-rays : stars;
D O I：
10.1093/pasj/57.3.L17
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We try to understand the quasi-periodic oscillations (QPOs) in low-mass neutron-star and black-hole X-ray binaries by a resonance model in warped disks with precession. Our main concern is high-frequency QPOs, hectohertz QPOs, and horizontal-branch QPOs in the z Sources and the atoll sources, and the corresponding QPOs in black-hole X-ray binaries. Our resonance model can qualitatively, but systematically, explain these QPOs by regarding hectohertz QPOs as a precession of warp.
引用
收藏
页码：L17 / L20
页数：4
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