Very High Energy Gamma Rays from Young Pulsars and Supernova Remnants in the Southern Hemisphere

Details Very High Energy Gamma Rays from Young Pulsars and Supernova Remnants in the Southern Hemisphere Very High Energy Gamma Rays from Young Pulsars and Supernova Remnants in the Southern Hemisphere

Jul 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000apj...537..414c&link_type=abstract

The Astrophysical Journal, Volume 537, Issue 1, pp. 414-421.

Astronomy and Astrophysics

Astronomy

10

Gamma Rays: Observations, Pulsars: Individual (Vela Pulsar, Psr B1055-52, Psr J1105-6107, Psr J0537-6910, Psr B0540-69)

Scientific paper

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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