Speaker
Hanrong WU
(IHEP)
Description
We present the analysis of 4 year LHAASO data of the middle-aged SNR W44 and the massive mocecular gas complex that surrounds it. We confirm the presence of the extended gamma-ray structure located near the remnant. Based on the high-resolution gas maps, we demonstrate that gamma-ray structures are caused by the interaction of escaped relativistic particles with Moclecular Clouds。We argu that the revealed cosmic-ray "clouds" suggest an anisotropic character of the escape of high energy particles frem the shell.
Authors
Hanrong WU
(IHEP)
Prof.
Min Zha
(IHEP)
Prof.
Bin Zhang
(IHEP)
Prof.
Zhen Cao
(IHEP)
Felix Aharonian
