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Paper: Evolved Stars: What Happens to Activity Off the Main Sequence
Volume: 154, Cool Stars, Stellar Systems and the Sun: Tenth Cambridge Workshop
Page: 257
Authors: Strassmeier, K. G.; Fekel, F. C.; Gray, D. F.; Hatzes, A. P.; Schmitt, J. H. M. M.; Solanki, S. K.
Abstract: Magnetic activity on the main sequence has been well studied, in contrast to researches on sub-giants, giants, and supergiant stars. In this discussion we will address three main topics associated with activity in evolved stars: (1) rotation regimes for evolved stars; (2) rotation-activity relations in the H-R diagram; (3) polar spots.
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