Abstract
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. © Elsevier Science B.V.
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APA
Lasota, J. P. (2001). The disc instability model of dwarf novae and low-mass X-ray binary transients. New Astronomy Reviews. Elsevier. https://doi.org/10.1016/S1387-6473(01)00112-9
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