Very high energy gamma rays from PKS 2155-304

被引:183
作者
Chadwick, PM [1 ]
Lyons, K [1 ]
McComb, TJL [1 ]
Orford, KJ [1 ]
Osborne, JL [1 ]
Rayner, SM [1 ]
Shaw, SE [1 ]
Turver, KE [1 ]
Wieczorek, GJ [1 ]
机构
[1] Univ Durham, Sci Labs, Dept Phys, Durham DH1 3LE, England
关键词
BL Lacertae objects : individual (PKS 2155-304); galaxies : active; gamma rays : observations;
D O I
10.1086/306862
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The close X-ray-selected BL Lac PKS 2155-304 has been observed using the University of Durham Mark 6 very high energy (VHE) gamma-ray telescope during 1996 September/October/November and 1997 October/November, VHE gamma rays with energy more than 300 GeV were detected from this object with a time-averaged integral flux of (4.2 +/- 0.7(stat) +/- 2.0(sys)) x 10(-11) cm(-2) s(-1). There is evidence for VHE gamma-ray emission during our observations in 1996 September and 1997 October/November, with the strongest emission being detected in 1997 November, when the object was producing the largest flux ever recorded in high-energy X-rays and it was detected as a source of gamma rays of energy greater than 100 MeV. The VHE and X-ray fluxes show evidence of a correlation.
引用
收藏
页码:161 / 167
页数:7
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