A multiple γ-ray source associated with a new supernova remnant

Details A multiple γ-ray source associated with a new supernova remnant A multiple γ-ray source associated with a new supernova remnant

Apr 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aipc..510...69c&link_type=abstract

THE FIFTH COMPTON SYMPOSIUM. AIP Conference Proceedings, Volume 510, pp. 69-72 (2000).

Computer Science

Gamma-Ray Sources, Gamma-Ray Bursts, Supernova Remnants, Gamma-Ray, Cosmic Rays

Scientific paper

Only a few of the 170 unidentified EGRET sources cluster within small regions of less than 6° in the sky. Here we present observational evidence supporting the association of such a group of three neighboring γ-ray sources (3EG J1834-2803, 3EG J1847-3219, and 3EG J1850-2652) with a new supernova remnant discovered at radio wavelengths. Two of the sources are coincident with HI clouds, detected through 21-cm line observations, which seem to be overtaken by the expanding shell of the remnant. The discovery of this multiple γ-ray source has profound implications for the origin of the galactic cosmic rays. .

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