The hard X-ray spectrum of Cyg X-1 during the transition in November 1975
Abstract
WE wish to report an observation of the hard X-ray spectrum of Cyg X-1 during a transition to the high state in November 1975. The measurement was obtained with a balloon-borne X-ray detector in the 25-150 keV range. This third upward transition of Cyg X-1 in 1975 was also detected in the few-keV energy range by the Ariel V all-sky monitor (S. S. Holt, L. J. Kaluzienski, E. A. Boldt, and P. J. Serlemitsos, unpublished). Our high energy data seem to confirm the characteristic spectral time variation of Cyg X-1: a soft X-ray intensity increase is correlated with a decrease of the hard X-ray intensity. The similarity of Cyg X-1 and the transient source A0620-00 with respect to such spectral variation has been pointed out by Coe et al.1.
- Publication:
-
Nature
- Pub Date:
- October 1976
- DOI:
- 10.1038/263752a0
- Bibcode:
- 1976Natur.263..752S
- Keywords:
-
- Supergiant Stars;
- X Ray Sources;
- X Ray Spectra;
- X Ray Stars;
- Energy Spectra;
- Radiant Flux Density;
- Spectrum Analysis;
- Astrophysics