Results of X-ray and optical monitoring of Scorpius X-1 in 1970

Details Results of X-ray and optical monitoring of Scorpius X-1 in 1970 Results of X-ray and optical monitoring of Scorpius X-1 in 1970

Apr 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975apj...197..425m&link_type=abstract

Astrophysical Journal, vol. 197, Apr. 15, 1975, pt. 1, p. 425-441. Research sponsored by the U.S. Department of Defense and AEC

Astronomy and Astrophysics

Astronomy

23

Spaceborne Astronomy, Ubv Spectra, X Ray Sources, X Ray Stars, Light Curve, Optical Measurement, Satellite Observation, Scorpius Constellation, Vela Satellites, X Ray Astronomy

Scientific paper

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.

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