The long-term evolution of stellar activity
Solar and Stellar Astrophysics
2017-09-20 v1
Abstract
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.
Cite
@article{arxiv.1612.04587,
title = {The long-term evolution of stellar activity},
author = {Scott G. Gregory},
journal= {arXiv preprint arXiv:1612.04587},
year = {2017}
}
Comments
Invited review. Proceedings of IAUS 328: Living around Active Stars (Maresias, Brazil, October 2016). 12 pages, 8 figures