Hostname: page-component-586b7cd67f-gb8f7 Total loading time: 0 Render date: 2024-11-30T07:24:18.469Z Has data issue: false hasContentIssue false
  • English
  • Français

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

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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