X-Ray Variability of the Am-Herculis Star CW1103+254
Abstract
The AM Her star CW1103+254 was observed with the low-energy and the medium-energy instruments of EXOSAT on 3 occasions for a total of 10.5 orbital cycles. Both, soft and hard X-rays from CW1103+254 were detected. We report preliminary results on the time variability of the X-ray emission on time scales from 1 minute to 1 month.
- Publication:
-
Space Science Reviews
- Pub Date:
- February 1985
- DOI:
- 10.1007/BF00212877
- Bibcode:
- 1985SSRv...40..139B
- Keywords:
-
- Stellar Spectrophotometry;
- Variable Stars;
- X Ray Sources;
- Emission Spectra;
- Exosat Satellite;
- Light Curve;
- Periodic Variations;
- Spectral Energy Distribution;
- Temporal Distribution;
- Astrophysics