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Chromospheres of Luminous Cool Stars

Published online by Cambridge University Press:  27 October 2016

A. K. Dupree*
Affiliation:
Harvard-Smithsonian Center for Astrophysics 60 Garden St., Cambridge, MA 02138, USA email: adupree@cfa.harvard.edu
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Abstract

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Direct ultraviolet imaging and spectroscopy of Alpha Orionis (Betelgeuse) reveals variable chromospheric structures and mass motions. Spectroscopy also demonstrates the changes of wind opacity, speeds, and mass loss in luminous stars. Cool stars have complex chromospheres that need to be considered in construction of stellar atmospheric models and subsequent spectral analyses.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2016 

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