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Pulsation and mass loss across the H-R diagram: From OB stars to Cepheids to red supergiants

Published online by Cambridge University Press:  18 February 2014

Hilding R. Neilson
Hilding R. Neilson*
Affiliation:
Department of Physics & Astronomy, East Tennessee State University, PO Box 70300, Johnson City, TN 37614, USA email: [email protected]
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Abstract

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Both pulsation and mass loss are commonly observed in stars and are important ingredients for understanding stellar evolution and structure, especially for massive stars. There is a growing body of evidence that pulsation can also drive and enhance mass loss in massive stars and that pulsation-driven mass loss is important for stellar evolution. In this review, I will discuss recent advances in understanding pulsation-driven mass loss in massive main-sequence stars, classical Cepheids and red supergiants and present some challenges remaining.

Keywords

circumstellar matterstars: evolutionstars: mass lossCepheids
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 9 , Symposium S301: Precision Asteroseismology , August 2013 , pp. 205 - 212
Copyright
Copyright © International Astronomical Union 2014 

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