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Active OB Stars - an introduction

Published online by Cambridge University Press:  12 July 2011

Dietrich Baade ,
Thomas Rivinius ,
Stanislas Štefl  and
Christophe Martayan
Dietrich Baade
Affiliation:
European Organisation for Astronomical Research in the Southern Hemisphere, Karl-Schwarzschild-Str. 2, 85748 Garching. b. München, Germany email: [email protected]
Thomas Rivinius
Affiliation:
European Organisation for Astronomical Research in the Southern Hemisphere, Casilla 19001, Santiago 19, Chile email: [email protected], [email protected], and [email protected]
Stanislas Štefl
Affiliation:
European Organisation for Astronomical Research in the Southern Hemisphere, Casilla 19001, Santiago 19, Chile email: [email protected], [email protected], and [email protected]
Christophe Martayan
Affiliation:
European Organisation for Astronomical Research in the Southern Hemisphere, Casilla 19001, Santiago 19, Chile email: [email protected], [email protected], and [email protected]
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Abstract

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Identifying seven activities and activity-carrying properties and nine classes of Active OB Stars, the OB Star Activity Matrix is constructed to map the parameter space. On its basis, the occurrence and appearance of the main activities are described as a function of stellar class. Attention is also paid to selected combinations of activities with classes of Active OB Stars. Current issues are identified and suggestions are developed for future work and strategies.

Keywords

stars: activitystars: binariesstars: circumstellar matterstars: early-typestars: emission-lineBestars: magnetic fieldsstars: mass lossstars: oscillationsstars: rotation
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 6 , Symposium S272: Active OB stars: structure, evolution, mass loss, and critical limits , July 2010 , pp. 1 - 13
Copyright
Copyright © International Astronomical Union 2011

References

On purpose, this paper does not provide any references: What is not expanded on in the following papers probably does not matter for the scope of this Symposium.Google Scholar