Discrete sources of gamma radiation, supernova remnants and pulsars

An attempt to identify detected by present discrete gamma radiation sources (Esub(γ) approximately equal to 108 eV) with known residuals of supernova flares is undertaken. An analysis of gamma source catalogue shows that most part (70%) of detected discrete gamma radiation sources may be identified with known residuals of sUpernova flares. Supernova residuals being identified have a low spectral index α < or approximately 0.3. Such objects, probably, contain a pulsar with a relatively large magnetic field. It is possible that supernovae 185g and 393g are related to gamma sources. There are not less than 150 similar gamma sources in Galaxy which contribute significantly into diffuse gamma radiation of a galactic disc