STUDY OF CYGNUS-X-3 AT ULTRAHIGH ENERGIES DURING THE 1989 RADIO OUTBURSTS

被引：5

作者：

ALEXANDREAS, DE

ALLEN, RC

BERLEY, D

BILLER, SD

BURMAN, RL

CADY, R

CHANG, CY

DINGUS, BL

DION, GM

ELLSWORTH, RW

GOODMAN, JA

HAINES, TJ

HOFFMAN, CM

LLOYDEVANS, J

LU, XQ

NAGLE, DE

POTTER, ME

SANDBERG, VD

STARK, MJ

TALAGA, RL

VISHWANATH, PR

YODH, GB

ZHANG, W

机构：

[1] UNIV MARYLAND,COLLEGE PK,MD 20742

[2] UNIV CALIF LOS ALAMOS SCI LAB,LOS ALAMOS,NM 87545

[3] UNIV NOTRE DAME,NOTRE DAME,IN 46556

[4] GEORGE MASON UNIV,FAIRFAX,VA 22030

来源：

PHYSICAL REVIEW LETTERS | 1990年 / 64卷 / 25期

关键词：

D O I：

10.1103/PhysRevLett.64.2973

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

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%-confidence-level limit of 3.0×10-13 cm-2 s-1 is placed on the flux above 50 TeV during the period from 15 May to 31 July 1989. © 1990 The American Physical Society.

引用

页码：2973 / 2975

页数：3

共 17 条

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