Seminar Title:	Discovery of TeV Supernova Remnant
Speaker:	Prof. Tian, WW
Affiliation:	(NAOC,CAS)
When:	Wednesday Morning, May. 18th, 10:30 a.m
Where:	Room 517, Office Block, 2 West Beijing Road (PMO, CAS)
	Welcome to Attend
	( PMO Academic Committee & Academic Circulating committee)

　

　 Abstract　　

　Seeking TeV sources' Galactic counterparts in lower energywavebands 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.