Abstract： Using observation data of the Tibet air shower array in different periods, a region with the highest excess of 4.4σ in the multi-TeV was detected from the SNR G40.5-0.5 direction, although statistically insignificant yet. The position of the highest excess is located around the EGRET unidentified source 3EG J1903+0550.
(Molecular clouds, H2 clouds, dense clouds, and dark clouds)
引用本文:
ZHANG Ji-Long;TAN You-Hen;LU Hong;WANG Hui. Search for the Multi-TeV Gamma Rays from the Shell-Like SNR G40.5-0.5 Using the Tibet Air Shower Array[J]. 中国物理快报, 2005, 22(6): 1560-1562.
ZHANG Ji-Long, TAN You-Hen, LU Hong, WANG Hui. Search for the Multi-TeV Gamma Rays from the Shell-Like SNR G40.5-0.5 Using the Tibet Air Shower Array. Chin. Phys. Lett., 2005, 22(6): 1560-1562.
2005, Vol. 22 
