VHE gamma rays from PSR B1706-44

被引：0

作者：

Chadwick, PM ^{[1
]}

Dickinson, MR ^{[1
]}

Dipper, NA ^{[1
]}

Holder, J ^{[1
]}

Kendall, TR ^{[1
]}

McComb, TJL ^{[1
]}

Orford, KJ ^{[1
]}

Osborne, JL ^{[1
]}

Rayner, SM ^{[1
]}

Roberts, ID ^{[1
]}

Shaw, SE ^{[1
]}

Turver, KE ^{[1
]}

机构：

[1] Univ Durham, Dept Phys, Durham DH1 3LE, England

来源：

PROCEEDINGS OF THE FOURTH COMPTON SYMPOSIUM, PTS 1 AND 2: PT 1: THE COMPTON OBSERVATORY IN REVIEW; PT 2: PAPERS AND PRESENTATIONS | 1997年 / 410期

关键词：

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Observations made with the University of Durham Mark 6 atmospheric Cerenkov telescope confirm that PSR B1706-44 is a VHE gamma-ray emitter. The gamma-ray flux has been measured at 250 GeV, and suggests a spectral dope that is consistent with extrapolation from the sub-10 GeV region. There is no indication from our dataset that the VHE gamma-rays are pulsed, in contrast to the findings at < 20 GeV, which indicate that 100% of the flux is pulsed.

引用

页码：612 / 616

页数：5

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