Discovery of radio pulsations from the X-ray pulsar in the supernova remnant G320.4-1.2

Details Discovery of radio pulsations from the X-ray pulsar in the supernova remnant G320.4-1.2 Discovery of radio pulsations from the X-ray pulsar in the supernova remnant G320.4-1.2

Nov 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982apj...262l..31m&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 262, Nov. 15, 1982, p. L31-L33.

Astronomy and Astrophysics

Astronomy

75

Pulsars, Radio Sources (Astronomy), Supernova Remnants, X Ray Sources, Pulse Duration, Temporal Distribution

Scientific paper

A radio counterpart to the X-ray pulsar discovered by Seward and Harnden in the supernova remnant G320.4-1.2 (MSH 15-52) has been detected. The radio observations confirm the very large period derivative indicated by the X-ray data. This implies that the object is not a member of a binary system and hence is an isolated pulsar similar in some ways to the Crab pulsar. Association of the pulsar and the supernova remnant is supported by the observed pulsar dispersion measure.

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