X-ray variability of cool stars: Magnetic activity and accretion
B. Stelzer (INAF - Osservatorio Astronomico di Palermo, Italy)
TL;DR
This paper reviews X-ray variability in cool stars, emphasizing magnetic activity and accretion, highlighting the contributions of XMM-Newton and prospects for future research in this area.
Contribution
It summarizes recent findings on X-ray variability in late-type stars and discusses the capabilities of XMM-Newton for advancing this research.
Findings
X-ray variability linked to magnetic activity and accretion in cool stars
XMM-Newton has significantly advanced understanding of stellar X-ray emissions
Future studies will benefit from improved observational techniques
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.
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