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Next generation model atmospheres

Published online by Cambridge University Press:  25 May 2016

Eugene H. Avrett
Eugene H. Avrett*
Affiliation:
Harvard-Smithsonian Center for Astrophysics 60 Garden Street, Cambridge, MA 02138, USA eavrett@cfa.harvard.edu

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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