In this paper we discuss numerical methods and algorithms for the solution of NLTE stellar atmosphere problems involving expanding atmospheres, e.g., found in novae, supernovae and stellar winds. We show how a scheme of nested iterations can be used to reduce the high dimension of the problem to a n
Structure of the expanding atmosphere of P Cygni
✍ Scribed by K. Avcioğlu
- Publisher
- Springer Netherlands
- Year
- 1984
- Tongue
- English
- Weight
- 619 KB
- Volume
- 106
- Category
- Article
- ISSN
- 0004-640X
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