Identification of the fast, high galactic latitude X-ray transient A 0000+28 with the RS CVn system HD 224085.
Abstract
We identify the fast, high galactic latitude X-ray transient A 0000+28 (=3A 2355+284) with HD 224085, a known RSCVn system. This strengthens the suggestion that RS CVn systems are responsible for a significant fraction of this class of X-ray transient. The hard X-ray flares provide further data relevant to the interpretation of these systems by analogy to solar phenomena.
- Publication:
-
Monthly Notices of the Royal Astronomical Society
- Pub Date:
- July 1981
- DOI:
- 10.1093/mnras/196.2.95
- Bibcode:
- 1981MNRAS.196...95S
- Keywords:
-
- Flare Stars;
- Stellar Luminosity;
- Stellar Radiation;
- X Ray Sources;
- Ariel 5 Satellite;
- Binary Stars;
- Light Curve;
- Stellar Coronas;
- X Ray Stars;
- Astronomy