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Next generation model atmospheres
Published online by Cambridge University Press: 25 May 2016
Abstract
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Continued progress in the physical interpretation of solar and stellar observations, the increased speed of computing now available, and new highly efficient numerical procedures have all led to significant advances in stellar atmospheric modeling. This review attempts to summarize recent progress in the field and to describe the many interrelated physical processes that should be taken into account in next-generation modeling programs.
- Type
- Session V: “Next Generation Model Atmospheres”
- Information
- Symposium - International Astronomical Union , Volume 176: Stellar Surface Structure , 1996 , pp. 503 - 518
- Copyright
- Copyright © Kluwer 1996
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