Coronal activity with XMM-Newton and Chandra
Beate Stelzer
TL;DR
This paper reviews recent advances in stellar coronal studies using XMM-Newton and Chandra, focusing on the solar-stellar connection, dynamo regimes, and X-ray emissions from pre-main sequence stars.
Contribution
It provides a concise overview of recent discoveries in stellar X-ray astronomy, emphasizing new diagnostics and key topics in the field.
Findings
Insights into the solar-stellar connection
Understanding of coronae in dynamo limiting regimes
X-ray emission characteristics of pre-main sequence stars
Abstract
XMM-Newton and Chandra have greatly deepened our knowledge of stellar coronae giving access to a variety of new diagnostics such that nowadays a review of stellar X-ray astronomy necessarily must focus on a few selected topics. Attempting to provide a limited but representative overview of recent discoveries I discuss three subjects: the solar-stellar connection, the nature of coronae in limiting regimes of stellar dynamos, and "hot topics" on X-ray emission from pre-main sequence stars.
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