A possible RS Canum Venaticorum system in the Coma star cluster.
Abstract
The double-lined spectroscopic binary T111 (HD 108102) in the Coma cluster of stars has many of the characteristics of RS Canum Venaticorum systems. It is the only RS Canum Venaticorum-type system known to be a member of a star cluster. Further observations at X-ray, optical and radio wavelengths are suggested.
- Publication:
-
The Astrophysical Journal
- Pub Date:
- June 1979
- DOI:
- 10.1086/182967
- Bibcode:
- 1979ApJ...230L..87B
- Keywords:
-
- Binary Stars;
- Star Clusters;
- Stellar Spectrophotometry;
- Optical Emission Spectroscopy;
- Radio Astronomy;
- X Ray Astronomy;
- Astrophysics;
- Open Clusters:RS CVn Stars