Pulsar Ejection in Supernova Events

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Scientific paper

ALTHOUGH pulsar formation is generally attributed to supernova events, only two pulsars are associated convincingly with known supernova remnants (the Crab Nebula and Vela). Other pulsars are close enough to remnants to suggest association1, but only if they are moving away from the remnant at velocities of the order of 103 km/s. Another problem seems to be that a supernova core may well be too massive to form a gravitationally stable object2 (for example a ``neutron star''), and gravitationally collapsing objects (``black holes'') do not presently seem promising candidates to be pulsars.

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