High energy X-ray and radio studies of Scorpius X-1

Details High energy X-ray and radio studies of Scorpius X-1 High energy X-ray and radio studies of Scorpius X-1

Apr 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apj...237..148c&link_type=abstract

Astrophysical Journal, Part 1, vol. 237, Apr. 1, 1980, p. 148-153.

Other

7

Binary Stars, Oso-8, Radio Waves, Scorpius Constellation, Stellar Spectrophotometry, X Ray Sources, Periodic Variations, Radiant Flux Density, Spectrum Analysis, X Ray Spectra

Scientific paper

The results from extended high energy X-ray observations of Scorpius X-1 from the OSO 8 satellite are reported. The source was observed for a total of 15 days in 1975, 1977, and 1978. Simultaneous 10.7 GHz and 4.75 GHz radio data were obtained during the 1978 observation, and low energy X-ray data during the 1975 and 1978 observations. Detailed studies of the data reveal a lack of any correlation between the high energy X-rays and the other energy ranges. A 3 sigma upper limit of 22% was obtained for any modulation of the high energy flux with the binary period. No high energy tail was observed at any time.

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