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

Published 2010-12-07Version 1

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/).