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Evolution of Stellar Magnetic Fields

Published online by Cambridge University Press:  05 March 2015

Manuel Güdel
Manuel Güdel*
Affiliation:
Department of Astrophysics, University of Vienna, Türkenschanzst. 17, 1180 Vienna, Austria email: manuel.guedel@univie.ac.at
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Abstract

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Stellar magnetic fields can reliably be characterized by several magnetic activity indicators, such as X-ray or radio luminosity. Physical processes leading to such emission provide important information on dynamic processes in stellar atmospheres and magnetic structuring.

Keywords

Stars: activitystars: coronaestars: flarestars: magnetic fields
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 10 , Highlights H16: Highlights of Astronomy , August 2012 , pp. 90 - 91
Copyright
Copyright © International Astronomical Union 2015 

References

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