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Title:
Very High Energy Gamma Rays from Young Pulsars and Supernova Remnants in the Southern Hemisphere
Authors:
Chadwick, P. M.; Lyons, K.; McComb, T. J. L.; Orford, K. J.; Osborne, J. L.; Rayner, S. M.; Shaw, S. E.; Turver, K. E.
Affiliation:
AA(Department of Physics, Rochester Building, Science Laboratories, University of Durham, Durham, DH1 3LE, UK; ), AB(Department of Physics, Rochester Building, Science Laboratories, University of Durham, Durham, DH1 3LE, UK), AC(Department of Physics, Rochester Building, Science Laboratories, University of Durham, Durham, DH1 3LE, UK), AD(Department of Physics, Rochester Building, Science Laboratories, University of Durham, Durham, DH1 3LE, UK; Present address: Department of Physics and Astronomy, Southampton University, Highfield, Southampton SO17 1BJ, UK), AE(Department of Physics and Astronomy, Southampton University, Highfield, Southampton SO17 1BJ, UK), AF(Department of Physics and Astronomy, Southampton University, Highfield, Southampton SO17 1BJ, UK), AG(Department of Physics and Astronomy, Southampton University, Highfield, Southampton SO17 1BJ, UK), AH(Department of Physics, Rochester Building, Science Laboratories, University of Durham, Durham, DH1 3LE, UK)
Publication:
The Astrophysical Journal, Volume 537, Issue 1, pp. 414-421. (ApJ Homepage)
Publication Date:
07/2000
Origin:
UCP
ApJ Keywords:
Gamma Rays: Observations, pulsars: individual (Vela pulsar, PSR B1055-52, PSR J1105-6107, PSR J0537-6910, PSR B0540-69)
DOI:
10.1086/309014
Bibliographic Code:
2000ApJ...537..414C

Abstract

Observations have been made with the University of Durham Mark 6 telescope of a number of southern hemisphere supernova remnants and young pulsars (Vela pulsar, PSR B1055-52, PSR J1105-6107, PSR J0537-6910, and PSR B0540-69). No very high energy gamma-ray emission, either steady or pulsed, has been detected from these objects. The implications of these results for theories of high-energy gamma-ray production in plerions and young pulsars are discussed.
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