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Constraining Stellar Winds of Young Sun-like Stars

Published online by Cambridge University Press:  07 August 2014

Colin P. Johnstone ,
Theresa Lüftinger ,
Manuel Güdel  and
Bibiana Fichtinger
Colin P. Johnstone
Affiliation:
University of Vienna, Department of Astronomy, Türkenschanzstrasse 17, 1180 Vienna, Austria
Theresa Lüftinger
Affiliation:
University of Vienna, Department of Astronomy, Türkenschanzstrasse 17, 1180 Vienna, Austria
Manuel Güdel
Affiliation:
University of Vienna, Department of Astronomy, Türkenschanzstrasse 17, 1180 Vienna, Austria
Bibiana Fichtinger
Affiliation:
University of Vienna, Department of Astronomy, Türkenschanzstrasse 17, 1180 Vienna, Austria
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Abstract

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As part of the project Pathways to Habitability (http://path.univie.ac.at/), we study the properties of the stellar winds of low-mass and Sun-like stars, and their influences on the atmospheres of potentially habitable planets. For this purpose, we combine mapping of stellar magnetic fields with magnetohydrodynamic wind models.

Keywords

stars: windsoutflowsstars: mass lossstars: magnetic fieldsMHD
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 9 , Symposium S302: Magnetic Fields throughout Stellar Evolution , August 2013 , pp. 243 - 244
Copyright
Copyright © International Astronomical Union 2014 

References

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