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arXiv · 1012.1626

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

Jan Forbrich·Scott J. Wolk·Manuel Güdel·Arnold Benz·Rachel Osten·Jeffrey L. Linsky·Margaret McLean·Laurent Loinard·Edo Berger
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Abstract

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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Jan Forbrich, Scott J. Wolk, Manuel Güdel, Arnold Benz, Rachel Osten, Jeffrey L. Linsky, Margaret McLean, Laurent Loinard, Edo Berger. 2010-12-07. The Radio-X-ray Relation in Cool Stars: Are we headed toward a divorce?. https://arxiv.org/abs/1012.1626

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