Published April 12, 2000 | Version v1
Journal article

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

  • 1. Max-Planck-Institut fuer extraterrestrische Physik, Postfach 1603, 85740 Garching (Germany)
  • 2. SRON, Sorbonnelaan 2, 3584 CA Utrecht (Netherlands)
  • 3. CESR-CNRS/UPS, 9, av. du Colonel-Roche, 31028 Toulouse Cedex (France)
  • 4. Space Science Center, University of New Hampshire, Durham, New Hampshire 03824 (United States)
  • 5. Astrophysics Division, ESTEC, ESA, 2200 AG Noordwijk (Netherlands)

Description

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

Additional details

Identifiers

Publishing Information

Journal Title
AIP Conference Proceedings
Journal Volume
510
Journal Issue
1
Journal Page Range
p. 49-53
ISSN
0094-243X
CODEN
APCPCS

Conference

Title
5. Compton symposium on gamma-ray astronomy
Dates
15-17 Sep 1999
Place
Portsmouth, NH (United States)

Optional Information

Notes
(c) 2000 American Institute of Physics.