## 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
Supersoft X-ray sources
✍ Scribed by F. Haberl
- Publisher
- John Wiley and Sons
- Year
- 2010
- Tongue
- English
- Weight
- 43 KB
- Volume
- 331
- Category
- Article
- ISSN
- 0004-6337
No coin nor oath required. For personal study only.
✦ Synopsis
Abstract
The workshop “Supersoft X‐ray Sources – New Developments” brought together observers and theoretician to discuss the present status and unsolved problems of supersoft source research. A large part of the workshop was devoted to optical novae and their supersoft state. Large samples of supersoft X‐ray sources were presented from nearby galaxies, as well as extensive monitoring campaigns ofbright individual sources. The theoretical modelling oflight curves and high‐resolution X‐ray spectra are well underway, but details are often not yet understood (© 2010 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)
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