Crab Nebula Pulsar NP 0532

Details Crab Nebula Pulsar NP 0532 Crab Nebula Pulsar NP 0532

Feb 1969

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1969natur.221..453c&link_type=abstract

Nature, Volume 221, Issue 5179, pp. 453-454 (1969).

Physics

74

Scientific paper

BECAUSE of the conjecture that pulsars are neutron stars, which are possibly produced in supernova events, the possible association of pulsars with supernova remnants is of great interest. Staelin and Reifenstein recently reported1 the discovery of two pulsed radio sources near the Crab nebula, which is the remnant of the supernova observed by the Chinese in AD 1054. Pulses from both sources were described as very sporadic, and no periodic phenomena were evident.

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