Results of X-ray and optical monitoring of Scorpius X-1 in 1970.
Abstract
Scorpius X-1 was monitored at optical and X-ray wavelengths from 1970 April 26 to 1970 May 20. The optical observations were made at six observatories around the world, and the X-ray observations were made by the Vela satellites. There was a tendency for the object to show greater variability in X-ray emission when the object was optically bright. The intensity histograms for both the optical and X-ray observations are discussed, as well as periodic variations in the optical intensity.
- Publication:
-
The Astrophysical Journal
- Pub Date:
- April 1975
- DOI:
- 10.1086/153528
- Bibcode:
- 1975ApJ...197..425M
- Keywords:
-
- Spaceborne Astronomy;
- Ubv Spectra;
- X Ray Sources;
- X Ray Stars;
- Light Curve;
- Optical Measurement;
- Satellite Observation;
- Scorpius Constellation;
- Vela Satellites;
- X Ray Astronomy;
- Astronomy