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The disc instability model of dwarf novae and low-mass X-ray binary transients

被引：802
作者：
Lasota, JP [1 ]
机构：
[1] Inst Astrophys, F-75014 Paris, France
来源：
NEW ASTRONOMY REVIEWS | 2001年 / 45卷 / 07期
关键词：
accretion discs; instabilities; dwarf novae; X-ray binaries; X-ray transients;
D O I：
10.1016/S1387-6473(01)00112-9
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The disc instability model which is supposed to describe outbursts of dwarf nova and low-mass X-ray binary transient systems is presented and reviewed in detail. Various deficiencies of the model are pointed out and various remedies and generalizations are presented and discussed. (C) 2001 Elsevier Science B.V. All rights reserved.
引用
收藏
页码：449 / 508
页数：60
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