期刊
NEW ASTRONOMY REVIEWS
卷 45, 期 7, 页码 449-508出版社
ELSEVIER SCI LTD
DOI: 10.1016/S1387-6473(01)00112-9
关键词
accretion discs; instabilities; dwarf novae; X-ray binaries; X-ray transients
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.
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