High Energy Gamma-Ray Pulsars

dc.contributor.author	Ramanamurthy, P. V
dc.date.accessioned	2008-04-21T06:47:07Z
dc.date.available	2008-04-21T06:47:07Z
dc.date.issued	1997
dc.identifier.citation	BASI, Vol. 25, No. 2, pp. 193 - 207	en
dc.identifier.uri	http://hdl.handle.net/2248/2234
dc.description.abstract	To date we know the existence of six high energy gamma-ray (HEGR) pulsars and a possible seventh candidate, besides a solitary low energy gamma-ray pulsar. In this paper, we briefly summarize the observations on the seven HEGR pulsars. We will then examine, treating all the HEGR pulsars as a 'population', if there is any emerging trend in their properties and try to compare the results with theoretical predictions	en
dc.format.extent	1368260 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1997BASI...25..193R	en
dc.subject	Gamma-rays	en
dc.subject	Pulsars	en
dc.subject	High Energy Interactions	en
dc.subject	Radio Astronomy	en
dc.title	High Energy Gamma-Ray Pulsars	en
dc.type	Article	en