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The Long-term Evolution of Stellar Activity by Gregory, Scott G. is a scholarly article available to read on EtoBox.

What is The Long-term Evolution of Stellar Activity about?

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.

Author

Gregory, Scott G.

Published

2016

Language

EN