Astronomy and Astrophysics – Astronomy
Scientific paper
Aug 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....1...95h&link_type=abstract
In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 1 p 95-98 (SEE N85-33902 22-93)
Astronomy and Astrophysics
Astronomy
Cosmic Ray Showers, Cygnus Constellation, Gamma Ray Bursts, Rates (Per Time), X Ray Astronomy, Cos-B Satellite, Extraterrestrial Radiation, Galactic Radiation
Scientific paper
COS-B had Cyg X-3 within its field of view during 7 observation periods between 1975 and 1982 for in total approximately 300 days. In the skymaps (70 meV E 5000 meV) of the Cyg-X region produced for each of these observations and in the summed map, a broad complex structure is visible in the region 72 deg approximately less than 1 approximately less than 85 deg, approximately less than 5 deg. No resolved source structure is visible at the position of Cyg X-3, but a weak signal from Cyg X-3 could be hidden in the structured gamma-ray background. Therefore, the data has been searched for a 4.8 h timing signature, as well as for a source signal in the sky map in addition to the diffuse background structure as estimated from tracers of atomic and molecular gas.
Bennett Kevin
Bignami Giovanni F.
Bloemen Johannes Bernardus Gerhardus Maria
Buccheri Rosolino
Caraveo Patricia A.
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