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

页码：L17 / L20

页数：4

共 13 条

[1] A precise determination of black hole spin in GRO J1655-40 [J].