Upper limits on the cyclotron lines from HER X-1 as observed with OSO-8
Abstract
Observations of Her X-1 were obtained during its ON-state in September, 1977, with the high-energy X-ray detector on board OSO-8. Upper limits on the line fluxes at 60 and 135 keV based on these observations are above, and hence consistent with, the positive results reported by Trumper, et al from a balloon flight during the same time interval. A detailed analysis of the time-variable et al background spectrum suggests that the line emission, especially in the time-averaged spectrum of Her X-1 previously reported by other workers at 25, 60, and 135 keV, is due to instrumental effects. The spectrum obtained with OSO-8 in September, 1977, is considerably steeper than that observed in pre-1976 balloon flights. These results are consistent with the results obtained by Trumper showing a decrease in the effective temperature of Her X-1 between May, 1976, and September, 1977.
- Publication:
-
Gamma Ray Spectroscopy in Astrophysics
- Pub Date:
- August 1978
- Bibcode:
- 1978grsa.rept..371D
- Keywords:
-
- Astronomical Spectroscopy;
- Cyclotron Resonance;
- Emission Spectra;
- Hercules Nova;
- Line Spectra;
- Oso-8;
- X Ray Sources;
- Balloon-Borne Instruments;
- Temperature Gradients;
- X Ray Astronomy;
- X Ray Spectroscopy;
- Space Radiation