X-ray coronae of late-type stars: theoretical implications.
Abstract
The Einstein Observatory provided evidence for the ubiquity of coronae in late type stars. The hypothesis that loop-like structures, as seen in the solar corona, are also present in the coronae of other stars, is consistent with the available X-ray spectra.
- Publication:
-
X-ray Astronomy 1984
- Pub Date:
- 1985
- Bibcode:
- 1985xra..conf...17S
- Keywords:
-
- Late-Type Stars:Stellar Coronae;
- Stellar Coronae:Late-Type Stars;
- Stellar Coronae:X Rays;
- X Rays:Stellar Coronae