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The Crab nebula and pulsar in the MeV energy rangeThe imaging Compton Telescope (COMPTEL) is sensitive in the energy range of 0.75 to 30 MeV. COMPTEL observed the Crab several times during the Compton Gamma Ray Observatory (CGRO) sky survey and CGRO Phase II. Both the Crab pulsar and nebula are detected over the entire COMPTEL energy range. The phase-averaged energy spectra of the Crab Pulsar and Nebula are presented. The combined observations provide sufficient statistics for a phase-resolved analysis of the Crab pulsar spectrum.
Document ID
19950044472
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1016/0273-1177(94)00041-X
Authors
Much, R. (ESTEC Noordwijk, Netherlands)
Bennett, K. (ESTEC Noordwijk, Netherlands)
Buccheri, R. (IFCAI/CNR Palermo, Itlay, United States)
Busetta, M. (ESTEC Noordwijk, Netherlands)
Diehl, R. (MPI fuer Extraterrestrische Physik Garching, Germany)
Forrest, D. (Univ. of New Hampshire, Durham, NH US, United States)
Hermsen, W. (SRON-Utrecht Utrecht, Netherlands)
Kuiper, L. (SRON-Utrecht Utrecht, Netherlands)
Lichti, G. G. (MPI fuer Extraterrestrische Physik Garching, Germany)
Mcconnell, M. (Univ. of New Hampshire, Durham, NH US, United States)
Date Acquired
August 16, 2013
Publication Date
May 1, 1995
Publication Information
Publication: Advances in Space Research
Volume: 15
Issue: 5
ISSN: 0273-1177
Subject Category
Astronomy
Accession Number
95A76071
Funding Number(s)
CONTRACT_GRANT: NAS2-6645
CONTRACT_GRANT: DARA-50-QV-90-968
Distribution Limits
Public
Copyright
Other

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