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Atmospheric emission from hydrogen-shell-burning white dwarfs as supersoft X-ray sources

✍ Scribed by Toshiya Shimura


Publisher
John Wiley and Sons
Year
2000
Tongue
English
Weight
608 KB
Volume
315
Category
Article
ISSN
0035-8711

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Accreting white dwarfs as supersoft X-ra
✍ M. Kato 📂 Article 📅 2010 🏛 John Wiley and Sons 🌐 English ⚖ 274 KB 👁 2 views

## 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 (__Ṁ__~acc~ < a few × 10^–7^ M⊙yr^–1^), hydrogen nuclear burning is unstable and nova outbursts occur. A nova is a transient supersoft