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X-ray emission from isolated hot white dwarfs

✍ Scribed by John Heise

Publisher
Springer Netherlands
Year
1985
Tongue
English
Weight
715 KB
Volume
40
Category
Article
ISSN
0038-6308

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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