Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1930
Title: Gamma ray production in SNR's -contribution from photomeson process
Authors: Bhattacharya, S
Kaul, R. K
Kaul, C. L
Bhat, C. L
Keywords: Gamma ray;Photo-meson;Supernova Remnants(SNR)
Issue Date: 1999
Publisher: Astronomical Society of India
Citation: BASI, Vol. 27, No. 1, pp. 185 - 189
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.
URI: http://hdl.handle.net/2248/1930
???metadata.dc.relation.uri???: http://adsabs.harvard.edu/abs/1999BASI...27..185B
Appears in Collections:BASI Publications

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