An optical precursor to the recent soft X-ray outburst the black hole binary GRO J1655-40

被引：0

作者：

Orosz, JA ^{[1
]}

Remillard, RA ^{[1
]}

Bailyn, CD ^{[1
]}

McClintock, JE ^{[1
]}

机构：

[1] Penn State Univ, University Pk, PA 16802 USA

来源：

WILD STARS IN THE OLD WEST: PROCEEDINGS OF THE 13TH NORTH AMERICAN WORKSHOP ON CATACLYSMIC VARIABLES AND RELATED OBJECTS | 1997年 / 137卷

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D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We discuss the observation of an optical outburst that preceded the April 1996 X-ray outburst of GRO J1655-40 by approximate to 6 days. The onset of the optical brightening was earliest in I and latest in B, however the rate of increase was largest in B and smallest in I. The dependence of the onset times and rates of increase on the color strongly suggests an "outside-in" disturbance of the accretion disk. The substantial delay between the optical outburst and the X-ray outburst constrains models of the accretion flow in this system.

引用

页码：504 / 505

页数：2

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