The disc instability model of dwarf-novae and low-mass X-ray binary transients
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🌌 astro-ph
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modelbinarydiscinstabilitylow-masspresentedvariousx-ray
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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.
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