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Gamma-ray emission from young neutron starsThe emission models of Cheng et al. (1986) and Harding (1981) are employed to determine likely candidates for pulsed gamma-ray emission on the basis of recent radio data of pulsars. The recent detection of pulsed gamma rays from PSR 1951+32 lends observational support to the scenario of Cheng et al. which also suggests that PSR 1855+09 might be another excellent gamma-ray pulsar candidate. The possible contribution of young neutron stars to the diffuse high energy glow is also discussed.
Document ID
19930041009
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Hartmann, Dieter H. (NASA Headquarters Washington, DC United States)
Liang, Edison P. (Lawrence Livermore National Lab. Livermore, CA, United States)
Cordes, J. M. (Cornell Univ. Ithaca, NY, United States)
Date Acquired
August 16, 2013
Publication Date
January 1, 1991
Publication Information
Publication: In: High energy gamma-ray astronomy; Proceedings of the International Conference, Ann Arbor, MI, Oct. 2-5, 1990 (A93-25001 08-93)
Publisher: American Institute of Physics
Subject Category
Astrophysics
Accession Number
93A25006
Funding Number(s)
CONTRACT_GRANT: W-7405-ENG-48
Distribution Limits
Public
Copyright
Other

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