Physical Sciences: 80 MHz Observations of the Scorpius X-1 Source

Details Physical Sciences: 80 MHz Observations of the Scorpius X-1 Source Physical Sciences: 80 MHz Observations of the Scorpius X-1 Source

Nov 1971

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1971natur.234q.210s&link_type=abstract

Nature, Volume 234, Issue 5326, pp. 210 (1971).

Physics

2

Scientific paper

Andrew and Purton1 discovered a weak high frequency radio source, which they identified with the strong X-ray source Sco X-1. The identification was confirmed by Ables2, who also discovered significant changes in the source's flux density. A subsequent high resolution study of the region by Hjellming and Wade3 at 2,695 and 8,085 MHz showed clearly the presence of three closely spaced sources; the central source was found to be highly variable over a period of hours and was identified with the optical object associated with the X-ray source. It was noted that its flare emission tended to be considerably stronger at 2,695 MHz than at 8,085 MHz, with spectral indices of upto 1.5.

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