X-ray variability of cool stars: Magnetic activity and accretion
arXiv:1611.07794 · doi:10.1002/asna.201713330
Abstract
This article provides a review of X-ray variability from late-type stars with particular focus on the achievements of XMM-Newton and its potential for future studies in this field.
6 pages, to appear in Astronomische Nachrichten as part of the proceedings of "XMM-Newton: The Next Decade", held at ESAC, Madrid, Spain, 9-11 May 2016