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Atmospheres, magnetism, mass loss of red supergiant stars

Published online by Cambridge University Press:  24 July 2015

E. Josselin ,
J. Lambert ,
M. Aurière ,
P. Petit  and
N. Ryde
E. Josselin
Affiliation:
LUPM, Université Montpellier II, CNRS, France email: eric.josselin@univ-montp2.fr Department of Astronomy and Theoretical Physics, Lund Observatory, Sweden
J. Lambert
Affiliation:
Department of Astronomy and Theoretical Physics, Lund Observatory, Sweden
M. Aurière
Affiliation:
Université de Toulouse, UPS-OMP, Institut de Recherche en Astrophysique et Planétologie, Toulouse, France
P. Petit
Affiliation:
Université de Toulouse, UPS-OMP, Institut de Recherche en Astrophysique et Planétologie, Toulouse, France
N. Ryde
Affiliation:
Department of Astronomy and Theoretical Physics, Lund Observatory, Sweden
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Abstract

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Red supergiant stars (RSGs) are not only a key evolutionary stage of massive stars participating in the chemical evolution of galaxies, they also represent a fantastic and challenging laboratory of (magneto-)hydrodynamics. We present recent results and on-going research on mass loss, atmospheres, and polarimetric studies of RSGs that reveal a magnetic field of unknown origin. We discuss the potential interplay between these different processes.

Keywords

Polarizationstars: atmospheresstars: magnetic fieldsstars: mass losssupergiants
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 10 , Symposium S305: Polarimetry: From the Sun to Stars and Stellar Environments , December 2014 , pp. 299 - 300
Copyright
Copyright © International Astronomical Union 2015 

References

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