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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2234
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dc.contributor.authorRamanamurthy, P. V-
dc.date.accessioned2008-04-21T06:47:07Z-
dc.date.available2008-04-21T06:47:07Z-
dc.date.issued1997-
dc.identifier.citationBASI, Vol. 25, No. 2, pp. 193 - 207en
dc.identifier.urihttp://hdl.handle.net/2248/2234-
dc.description.abstractTo 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 predictionsen
dc.format.extent1368260 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/1997BASI...25..193Ren
dc.subjectGamma-raysen
dc.subjectPulsarsen
dc.subjectHigh Energy Interactionsen
dc.subjectRadio Astronomyen
dc.titleHigh Energy Gamma-Ray Pulsarsen
dc.typeArticleen
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