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Radiative Transfer in Dynamic Stellar Atmospheres
Published online by Cambridge University Press: 14 August 2015
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
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- Copyright
- Copyright © Reidel 1976
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