The Radio-X-ray Relation in Cool Stars: Are We Headed Toward a Divorce?
- Author(s)
- J. Forbrich, S. J. Wolk, M. Güdel, A. Benz, R. Osten, J. L. Linsky, M. McLean, L. Loinard, E. Berger
- Abstract
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(s)
- Department of Astrophysics
- Journal
- Astronomical Society of the Pacific Conference Series
- Volume
- 448
- Pages
- 455
- ISSN
- 1050-3390
- Publication date
- 12-2011
- Austrian Fields of Science 2012
- 103004 Astrophysics
- Portal url
- https://ucrisportal.univie.ac.at/en/publications/4ff6bcc4-33fb-499e-b0c6-e776e14e1bb5