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 |
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creator | 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 |
description | 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) |
doi_str_mv | 10.1103/PhysRevLett.64.2973 |
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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</creator><creatorcontrib>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</creatorcontrib><description>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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W</creatorcontrib><title>Study of Cygnus X-3 at ultrahigh energies during the 1989 radio outbursts</title><title>Physical review letters</title><addtitle>Phys Rev Lett</addtitle><description>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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L</au><au>CADY, R</au><au>CHANG, C. Y</au><au>DINGUS, B. L</au><au>DION, G. M</au><au>ELLSWORTH, R. W</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Study of Cygnus X-3 at ultrahigh energies during the 1989 radio outbursts</atitle><jtitle>Physical review letters</jtitle><addtitle>Phys Rev Lett</addtitle><date>1990-06-18</date><risdate>1990</risdate><volume>64</volume><issue>25</issue><spage>2973</spage><epage>2975</epage><pages>2973-2975</pages><issn>0031-9007</issn><eissn>1079-7114</eissn><coden>PRLTAO</coden><abstract>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)</abstract><cop>Ridge, NY</cop><pub>American Physical Society</pub><pmid>10041862</pmid><doi>10.1103/PhysRevLett.64.2973</doi><tpages>3</tpages></addata></record> |
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subjects | 640101 - Astrophysics & Cosmology- Cosmic Radiation 640102 - Astrophysics & Cosmology- Stars & Quasi-Stellar, Radio & X-Ray Sources Astronomy CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS COSMIC GAMMA BURSTS COSMIC RADIATION DATA ANALYSIS Earth, ocean, space ENERGY RANGE ENERGY SPECTRA Exact sciences and technology Gamma-ray sources gamma-ray bursts IONIZING RADIATIONS PRIMARY COSMIC RADIATION RADIATIONS SPECTRA Stellar systems. Galactic and extragalactic objects and systems. The universe TEV RANGE TIME DEPENDENCE Unidentified sources and radiation outside the solar system |
title | Study of Cygnus X-3 at ultrahigh energies during the 1989 radio outbursts |
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