作者: Yousaf M. Butt , Jorge A. Combi , Thomas M. Dame , Gustavo E. Romero , Diego F. Torres
DOI: 10.1016/S0370-1573(03)00201-1
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摘要: Abstract A review of the possible relationship between γ -ray sources and supernova remnants (SNRs) is presented. Particular emphasis given to analysis observational status problem cosmic ray acceleration at SNR shock fronts. All positional coincidences SNRs unidentified listed in Third EGRET Catalog low Galactic latitudes are discussed on a case by basis. For several particular interest, new CO( J =1−0) radio continuum maps shown, mass content surroundings determined. The contribution flux observed that might come from particles (particularly nuclei) locally accelerated fronts evaluated. We discuss prospects for future research this field remark possibilities observations with forthcoming instruments.