COMPTEL upper limits for the 56Co γ-rays from SN1998bu

Details COMPTEL upper limits for the 56Co γ-rays from SN1998bu COMPTEL upper limits for the 56Co γ-rays from SN1998bu

Apr 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aipc..510...49g&link_type=abstract

THE FIFTH COMPTON SYMPOSIUM. AIP Conference Proceedings, Volume 510, pp. 49-53 (2000).

Physics

Nuclear Physics

3

Supernovae, Nuclear Physics Aspects Of Novae, Supernovae, And Other Explosive Environments, Gamma-Ray, Observation And Data Reduction Techniques, Computer Modeling And Simulation

Scientific paper

The type Ia supernova SN 1998bu in M96 was observed by COMPTEL for a total of 88 days starting 17 days after the detection of the SN. A special mode improving the low-energy sensitivity was invoked. We obtained images in the 847 keV and 1238 keV lines of 56Co using an improved point-spread function for the low-energies. We do not detect SN1998bu. Sensitive upper limits at both energies constrain the standard supernova model for this event. .

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