The Radio-X-ray Relation in Cool Stars: Are We Headed Toward a Divorce?

Autor(en)

J. Forbrich, S. J. Wolk, M. Güdel, A. Benz, R. Osten, J. L. Linsky, M. McLean, L. Loinard, E. Berger

Abstrakt

This splinter session was devoted to reviewing our current knowledge of correlated X-ray and radio emission from cool stars in order to preparefor new large radio observatories such as the EVLA. A key interest wasto 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, theso-called Güdel-Benz relation. This article summarizes the contributions whereas the actual presentations can be accessed on the splinter website.

Organisation(en)

Institut für Astrophysik

Journal

Astronomical Society of the Pacific Conference Series

Band

448

Seiten

455

ISSN

1050-3390

Publikationsdatum

12-2011

ÖFOS 2012

103004 Astrophysik

Link zum Portal

https://ucrisportal.univie.ac.at/de/publications/4ff6bcc4-33fb-499e-b0c6-e776e14e1bb5