X-ray variability of cool stars: Magnetic activity and accretion

Author:

BSB. Stelzer
B. Stelzer

Preprint

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23 November 2016

preprint
Published by arXiv in arXiv

DOI:10.48550/arXiv.1611.07794

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.

Keywords

X-RAY VARIABILITY
MAGNETIC ACTIVITY
FUTURE STUDIES
COOL STARS
LATE-TYPE STARS
X-RAY
MAGNETIC
VARIABILITY
STARS
FIELD

All Related Versions

Version 1, 2016-11-23, ArXiv
Published version: Astronomische Nachrichten, 338 (2-3), 195.