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High-resolution observations of gamma-ray line emission from SN 1987A

Conference · · AIP Conf. Proc.; (United States)
OSTI ID:6921394
A balloon-borne gamma-ray spectrometer comprising an array of high-purity germanium (HPGE) detectors was flown from Alice Springs, Australia, on October 29--30--31, norminally 250 days after the observed neutrino pulse. High-resolution data, typically 2.5 keV at 1.33 MeV, for two transists of the supernova SN 1987A were obtained along with interspersed background data. A significant net flux of gamma rays with energy 847 keV was observed from the direction of SN 1987A on each transit. No prominent gamma-ray features were seen at other energies, although data analysis is still in progress. A preliminary estimate of the line flux at 847 keV is approx.5 x 10/sup -4/ photons cm/sup -2/ s/sup -1/ with statistical significance greater than three sigma. This line may be interpreted as emission from the first excited state of /sup 56/Fe due to the radioactive decay of /sup 56/Co, providing strong evidence for nucleosynthesis in the supernova. No emission was seen from the second excited state of /sup 56/Fe at 1238 keV. A preliminary upper limit for the 1238-keV line is approx.5 x 10/sup -4/ photons cm/sup -2/ s/sup -1/. The flux estimates may be considerably altered as the systematics of the experiment are better understood.
Research Organization:
Lockheed Palo Alto Research Laboratory, 3251 Hanover St., Palo Alto, CA 94304
OSTI ID:
6921394
Report Number(s):
CONF-871245-
Conference Information:
Journal Name: AIP Conf. Proc.; (United States) Journal Volume: 170:1
Country of Publication:
United States
Language:
English