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On the Stellar Rotation-Activity Connection

Published online by Cambridge University Press:  04 August 2017

Robert Rosner
Robert Rosner*
Affiliation:
Harvard-Smithsonian Center for Astrophysics Cambridge, MA 02138 USA

Abstract

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I discuss the connection between the rotation rate of late-type dwarf stars and their level of surface “activity” (as deduced from visible, UV, and X-ray observations) from both theoretical and observational perspectives.

Type
III. Theory of Stellar Magnetic Field Generation
Information
Symposium - International Astronomical Union , Volume 102: Solar and Stellar Magnetic Fields: Origins and Coronal Effects , 1983 , pp. 279 - 300
Copyright
Copyright © Reidel 1983 

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