The Radio-X-ray Relation in Cool Stars: Are we headed toward a divorce?

Details The Radio-X-ray Relation in Cool Stars: Are we headed toward a divorce? The Radio-X-ray Relation in Cool Stars: Are we headed toward a divorce?

2010-12-07

arxiv.org/abs/1012.1626v1

Astronomy and Astrophysics

Astrophysics

Solar and Stellar Astrophysics

12 pages, Cool Stars 16 splinter session summary, to appear in conference proceedings

Scientific paper

This Cool Stars 16 splinter session was devoted to reviewing our current knowledge of correlated X-ray and radio emission from cool stars in order to prepare for new large radio observatories such as the EVLA. A key interest was to discuss why the X-ray and radio luminosities of some cool stars are in clear breach of a correlation that holds for other active stars, the so-called G\"udel-Benz relation. This article summarizes the contributions whereas the actual presentations can be accessed on the splinter website (http://cxc.harvard.edu/cs16xrayradio/).

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