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Fluid instabilities around accreting X-ray sources

✍ Scribed by Y.-M. Wang

Book ID
103647572
Publisher
Elsevier Science
Year
1984
Tongue
English
Weight
188 KB
Volume
3
Category
Article
ISSN
0273-1177

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## Abstract I review various phenomena associated with mass‐accreting white dwarfs (WDs) in the view of supersoft X‐ray sources. When the mass‐accretion rate is low (__αΉ€__~acc~ < a few Γ— 10^–7^ MβŠ™yr^–1^), hydrogen nuclear burning is unstable and nova outbursts occur. A nova is a transient supersoft