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The long-term evolution of stellar activity

Published online by Cambridge University Press:  12 September 2017

Scott G. Gregory
Scott G. Gregory*
Affiliation:
School of Physics & Astronomy, University of St Andrews, St Andrews, KY16 9SS, U. K. email: [email protected]
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Abstract

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I review the evolution of low-mass stars with outer convective zones over timescales of millions-to-billions of years, from the pre-main sequence to solar-age, ~4.6 Gyr (Bahcall et al. 1995; Amelin et al. 2010), and beyond. I discuss the evolution of high-energy coronal and chromospheric emission, the links with stellar rotation and magnetism, and the emergence of the rotation-activity relation for stars within young clusters.

Keywords

stars: activitystars: chromospheresstars: coronaestars: evolutionstars: interiorsstars: late-typestars: magnetic fieldsstars: pre-main sequencestars: rotationX-rays: stars
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 12 , Symposium S328: Living Around Active Stars , October 2016 , pp. 252 - 263
Copyright
Copyright © International Astronomical Union 2017 

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