Mass and spin of GRS 1915+105 based on a resonance model of QPOs

被引：22

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 | 2004年 / 56卷 / 05期

关键词：

accretion; accretion disks; kiloherz quasi-periodic oscillations; relativity; stars : individual (GRS 1915+105); warps;

D O I：

10.1093/pasj/56.5.L25

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We demonstrate that the four high-frequency QPOs observed in GRS 1915 + 105 can be interpreted as the oscillation modes on disks that non-linearly and resonantly interact with a warp. The warp is assumed to be a low-frequency global pattern on the disk. This identification suggests that the relevant mass, M, and spin parameter, a, are M = 13-14 M-circle dot and a = 0-0.15.

引用

页码：L25 / L28

页数：4

共 13 条

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