Sco X-1 - a source of 300 GeV gamma rays

Details Sco X-1 - a source of 300 GeV gamma rays Sco X-1 - a source of 300 GeV gamma rays

Mar 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990nuphs..14..191b&link_type=abstract

Nuclear Physics B Proceedings Supplements, Volume 14, Issue 1, p. 191-195.

Physics

Nuclear Physics

Scientific paper

Observations have been made in 1988 and 1989 using the Narrabri VHE gamma ray telescope which each show evidence significant at > 3 σ level for a DC detection of 300 GeV gamma rays from Sco X-1. There are indications that the emission was modulated with the 0.787 d orbital period. No evidence for periodicity is found at or near the 2.92 or 4.53 ms periods suggested in the analyses of X-ray measurements.

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