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 VHE 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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