X-ray variability of cool stars: Magnetic activity and accretion
Solar and Stellar Astrophysics
2017-05-10 v1
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.
Cite
@article{arxiv.1611.07794,
title = {X-ray variability of cool stars: Magnetic activity and accretion},
author = {B. Stelzer},
journal= {arXiv preprint arXiv:1611.07794},
year = {2017}
}
Comments
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