EGRET Observations of Gamma-Ray Emission from Supernova Remnants
Abstract
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
- Publication:
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American Astronomical Society Meeting Abstracts #188
- Pub Date:
- May 1996
- Bibcode:
- 1996AAS...188.2806E