Coronal activity with XMM-Newton and Chandra
Sep, 200810 pages
Part of Proceedings, 15th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun (Cool Stars 15) : St. Andrews, Scotland, July 21-25, 2008, 190-199
Published in:
- AIP Conf.Proc. 1094 (2009) 1, 190-199
Contribution to:
- , 190-199
- Cool Stars 15
- Published: Feb 25, 2009
e-Print:
- 0809.4361 [astro-ph]
DOI:
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Abstract: (AIP)
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.- 97.10.Ex
- 78.70.En
- 97.80.Jp
- X-ray astronomy
- corona
- X-ray emission spectra
References(44)
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