题  目：高能宇宙线和超新星遗迹

报告人：田文武  教授(国家天文台)

摘  要：Seeking TeV sources' Galactic counterparts in lower energy wavebands could play a key role for us to understand the origin of TeV sources and distinguish different acceleration mechanisms for emitting TeV gamma-rays. Discovery of TeV Supernova Remnant (SNR) G353.6-0.7 likely provides the best case that an old SNR emits TeV gamma-rays. Distance measurements to Galactic SNRs are a challenging job. I will introduce an  improved method of distance measurement by HI and CO analysis, and show its applications to SNR/pulsar/TeV source systems.

时  间：2011年5月18日（星期三）上午10:30

地  点：（北京西路2号）紫台大楼517会议室

欢迎大家积极参与！

　　　　　　　　　　　　　　 紫金山天文台学术委员会学术交流工作委员会