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

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...

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Veröffentlicht in:Physical review letters 1990-06, Vol.64 (25), p.2973-2975
Hauptverfasser: ALEXANDREAS, D. E, ALLEN, R. C, GOODMAN, J. A, HAINES, T. J, HOFFMAN, C. M, LLOYD-EVANS, J, LU, X.-Q, NAGLE, D. E, POTTER, M. E, SANDBERG, V. D, STARK, M. J, TALAGA, R. L, BERLEY, D, BILLER, S. D, BURMAN, R. L, CADY, R, CHANG, C. Y, DINGUS, B. L, DION, G. M, ELLSWORTH, R. W
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Sprache:eng
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Zusammenfassung: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. (Author)
ISSN:0031-9007
1079-7114
DOI:10.1103/PhysRevLett.64.2973