Study of Cygnus X-3 at ultrahigh energies during the 1989 radio outbursts

Details Study of Cygnus X-3 at ultrahigh energies during the 1989 radio outbursts Study of Cygnus X-3 at ultrahigh energies during the 1989 radio outbursts

Jun 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990phrvl..64.2973a&link_type=abstract

Physical Review Letters (ISSN 0031-9007), vol. 64, June 18, 1990, p. 2973-2975. Research supported by Los Alamos National Labora

Astronomy and Astrophysics

Astronomy

6

Cosmic Ray Showers, Radio Bursts, Space Observations (From Earth), Stellar Flares, X Ray Binaries, Energy Spectra, Muons, Primary Cosmic Rays, Radio Astronomy, Scintillation Counters

Scientific paper

A unique feature of Cygnus X-3 is that, occasionally, it has large radio outbursts that begin very abruptly and last for several days. Several experiments in the past have claimed to observe signals above 1 TeV correlated with these radio bursts; the most recent bursts occurred in June and July 1989. No significant signal was observed by the CYGNUS experiment over time scales longer than a day during this time; a 90-percent confidence-level limit of 3.0 x 10 to the -13th/sq cm per sec is placed on the flux above 50 TeV during the period from May 15 to July 31, 1989.

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