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Radiative Transfer in Dynamic Stellar Atmospheres

Published online by Cambridge University Press:  14 August 2015

Richard I. Klein
Richard I. Klein*
Affiliation:
National Center for Atmospheric Research, Boulder, Colo., U.S.A.

Abstract

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In order to understand the Be star phenomenon, and move in directions away from ad hoc models, detailed calculations have been made that treat nonlinear hydrodynamics self-consistently with non-L.T.E. radiative transfer.

Type
Part IV: Line Formation in Expanding Atmospheres
Information
Symposium - International Astronomical Union , Volume 70: Be and Shell Stars , 1976 , pp. 313
Copyright
Copyright © Reidel 1976