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

May 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978stin...7928077c&link_type=abstract

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Radio Observation, Scorpius Constellation, X Ray Spectra, Digital Systems, Flux (Rate), Modulation, Photons, Standard Deviation, X Ray Sources, X Rays

Scientific paper

The results from extended high energy X-ray observations of Scorpius XR-1 from the OSO-8 satellite are reported here. 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. The data reveals a lack of any correlation between the high energy X-rays and the other energy ranges. A three standard deviation 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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