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Pulsating Stellar Atmospheres

  • Dimitar D. Sasselov
Conference paper
Part of the International Astronomical Union / Union Astronomique Internationale book series (IAUS, volume 189)

Abstract

We review the basic concepts, present state of theoretical models, and the future prospects for theory and observations of pulsating stellar atmospheres. Our emphasis is on radially pulsating cool stars, which dynamic atmospheres provide a general example for the differences with standard static model atmospheres.

Keywords

Radiative Transfer Stellar Atmosphere Cool Star Microturbulent Velocity Pulsate Star 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© Springer Science+Business Media Dordrecht 1997

Authors and Affiliations

  • Dimitar D. Sasselov
    • 1
  1. 1.Harvard-Smithsonian Center for AstrophysicsCambridgeUSA

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