Back to Search
Start Over
The Radio-X-ray Relation in Cool Stars: Are we headed toward a divorce?
- Publication Year :
- 2010
- Publisher :
- arXiv, 2010.
-
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/).<br />Comment: 12 pages, Cool Stars 16 splinter session summary, to appear in conference proceedings
- Subjects :
- Astrophysics - Solar and Stellar Astrophysics
Astrophysics::High Energy Astrophysical Phenomena
Astrophysics::Solar and Stellar Astrophysics
FOS: Physical sciences
Astrophysics::Cosmology and Extragalactic Astrophysics
Astrophysics::Galaxy Astrophysics
Solar and Stellar Astrophysics (astro-ph.SR)
Subjects
Details
- Database :
- OpenAIRE
- Accession number :
- edsair.doi.dedup.....5e1b57419906b54cf826f4f1717a25e5
- Full Text :
- https://doi.org/10.48550/arxiv.1012.1626