CTA 1 supernova remnant: A high energy gamma-ray source?

Details CTA 1 supernova remnant: A high energy gamma-ray source? CTA 1 supernova remnant: A high energy gamma-ray source?

May 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997aipc..410.1137b&link_type=abstract

The fourth compton symposium. AIP Conference Proceedings, Volume 410, pp. 1137-1141 (1997).

Mathematics

Probability

1

Supernova Remnants, Gamma-Ray, Gamma-Ray Sources, Gamma-Ray Bursts, Pulsars

Scientific paper

We discuss the excess gamma-ray emission seen from the direction of CTA 1, a supernova remnant, in the energy range of 100 MeV to 10 GeV with the EGRET instrument. The X-ray emission peak of CTA 1 seen by ROSAT falls within the 95% EGRET likelihood contour giving rise to the possibility that a central source is responsible for the high energy emission. We consider the probability that pulsars are responsible for most of the EGRET SNR candidate source emission.

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