Observations of the 4.8-hour variations of Cygnus X-3 above 7 keV from the OSO-7.
Abstract
Results of observations made (during the period from June 30 to July 5, 1972) of Cyg X-3 with the UCSD OSO-7 X-ray telescope in the range from about 7 to 100 keV. The 4.8-hour variation was detected in the 6.6-21.2 keV range, and the ratio of high intensity to mean intensity was 1.52 plus or minus 0.16. In the 21.2-97.8 keV range no 4.8-hour variation in phase with the 6.6-21.2 keV variation could be detected, and the ratio at the phase of high intensity to the mean intensity was 0.6 plus or minus 0.4.
- Publication:
-
The Astrophysical Journal
- Pub Date:
- September 1974
- DOI:
- 10.1086/153106
- Bibcode:
- 1974ApJ...192..691U
- Keywords:
-
- Radiant Flux Density;
- Satellite Observation;
- Spaceborne Astronomy;
- X Ray Sources;
- X Ray Spectra;
- Energy Spectra;
- Oso-7;
- Phase Shift;
- X Ray Telescopes;
- Astronomy