EGRET Observations of Gamma-Ray Emission from Supernova Remnants

Details EGRET Observations of Gamma-Ray Emission from Supernova Remnants EGRET Observations of Gamma-Ray Emission from Supernova Remnants

May 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aas...188.2806e&link_type=abstract

American Astronomical Society, 188th AAS Meeting, #28.06; Bulletin of the American Astronomical Society, Vol. 28, p.861

Astronomy and Astrophysics

Astronomy

Scientific paper

We have continued our analysis of data from EGRET observations of supernova remnants near the Galactic plane (Esposito et al. 1996). The integral intensities or upper limits have been determined, and spectra fitted when statistically justified. We have included cycle 4 data for some sources (e.g. IC443 and Monoceros). We will present our gamma-ray results and an interpretation based upon Galactic cosmic ray shock acceleration by supernova remnants. Esposito, J. A., Hunter, S. D., Kanbach, G. and Sreekumar, P, 20 April 1996, ApJ, in press

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