Gamma ray production in SNR's -contribution from photomeson process

dc.contributor.author	Bhattacharya, S
dc.contributor.author	Kaul, R. K
dc.contributor.author	Kaul, C. L
dc.contributor.author	Bhat, C. L
dc.date.accessioned	2007-10-27T11:46:15Z
dc.date.available	2007-10-27T11:46:15Z
dc.date.issued	1999
dc.identifier.citation	BASI, Vol. 27, No. 1, pp. 185 - 189	en
dc.identifier.uri	http://hdl.handle.net/2248/1930
dc.description.abstract	We estimate the integral γ-ray fluxes above 10 MeV photon energy, likely to result from neutral pion decay, following photomeson interactions between ultra-high energy protons accelerated in Supernova Remnants (SNR) and the background non-thermal X-ray photon field. Taking SN1006 as a test case, we find that the intergral fluxes in the TeV range are significantly lower than the experimentally reported values, indicating the ineffectiveness of the photo-meson interaction as a source of the reported Tev γ-ray signal from SNR.	en
dc.format.extent	331002 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/1999BASI...27..185B	en
dc.subject	Gamma ray	en
dc.subject	Photo-meson	en
dc.subject	Supernova Remnants(SNR)	en
dc.title	Gamma ray production in SNR's -contribution from photomeson process	en
dc.type	Article	en