Detection of Gamma Rays around 1 TeV from RX J0852.0–4622 by CANGAROO-II

Detection of Gamma Rays around 1 TeV from RX J0852.0–4622 by CANGAROO-II
复制标题

DOI：
10.1086/427980
复制
发表时间：
2004-12
期刊：
The Astrophysical Journal Letters
影响因子：
--
通讯作者：
H. Katagiri;R. Enomoto;L. Ksenofontov;M. Mori;Y. Adachi;A. Asahara;G. Bicknell;R. Clay;Y. Doi-Y
H. Katagiri;R. Enomoto;L. Ksenofontov;M. Mori;Y. Adachi;A. Asahara;G. Bicknell;R. Clay;Y. Doi-Y
中科院分区：
其他
文献类型：
--
作者：
H. Katagiri;R. Enomoto;L. Ksenofontov;M. Mori;Y. Adachi;A. Asahara;G. Bicknell;R. Clay;Y. Doi-Y

文献摘要

被引文献

相似文献

我们用CANGAROO-II成像大气切伦科夫望远镜从超新星遗迹RX J0852.0-4622（G266.2-1.2）中探测到了能量大于500 GeV的6 σ水平的γ射线辐射。在1 TeV时，其通量是Crab的0.12倍。信号中心与残骸西北边缘的X射线发射峰值一致。
We have detected gamma-ray emission at the 6 σ level at energies greater than 500 GeV from the supernova remnant RX J0852.0-4622 (G266.2-1.2) using the CANGAROO-II imaging atmospheric Cerenkov telescope. The flux was 0.12 times that of Crab at 1 TeV. The signal centroid is consistent with the peak of the X-ray emission in the northwest rim of the remnant.