Observations of discrete gamma ray sources with SAS-2

Details Observations of discrete gamma ray sources with SAS-2 Observations of discrete gamma ray sources with SAS-2

Nov 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974csgr.conf..273t&link_type=abstract

In ESRO The Context and Status of Gamma Ray Astronomy p 273-277 (SEE N75-25813 16-93)

Astronomy and Astrophysics

Astronomy

Galactic Radiation, Gamma Rays, Radiation Sources, Sas, Cosmic Rays, Crab Nebula, Flux Density, Photons, Pions, Radiation Distribution, Satellite Observation, Spiral Galaxies, Supernova Remnants, Vela Satellites

Scientific paper

Compact gamma ray sources centered on the Crab nebula and the Vela X supernova remnant are considered. An excess in the galactic radiation was observed in both regions. Data indicate that a large fraction of this flux is pulsed. The excess from the Vela region could reflect either a large-scale galactic feature, such as a superposition of spiral arm segments, or it could be associated with the Vela supernova remnant. Low-energy gamma ray bursts were observed in the SAS-2 anticoincidence shielding.

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