Preliminary results from COMPTEL on a search for gamma-ray line emission from SN 1991T

Details Preliminary results from COMPTEL on a search for gamma-ray line emission from SN 1991T Preliminary results from COMPTEL on a search for gamma-ray line emission from SN 1991T

Jan 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993a%26as...97..215l&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 97, no. 1, p. 215-218.

Astronomy and Astrophysics

Astronomy

5

Gamma Ray Spectra, Gamma Ray Telescopes, Line Spectra, Supernovae, Astronomical Models, Gamma Ray Observatory, Sky Surveys (Astronomy), Spectral Emission

Scientific paper

The COMPTEL experiment aboard the Compton Gamma-Ray Observatory is designed to image celestial gamma-radiation in the energy range from 0.7-30 MeV. With a field of view of 1 sr it is capable of locating strong point sources with an accuracy of better than 0.5 deg. From June 15 to 28, 1991 and a second time from October 3 to 17, 1991 the region containing the supernova SN 1991T was observed by COMPTEL. Here preliminary results from these observations are presented, with special attention to a search for gamma-ray line emission from the supernova.

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