A new, fast X-ray pulsar in the supernova remnant MSH 15-52

Details A new, fast X-ray pulsar in the supernova remnant MSH 15-52 A new, fast X-ray pulsar in the supernova remnant MSH 15-52

May 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982apj...256l..45s&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 256, May 15, 1982, p. L45-L47.

Astronomy and Astrophysics

Astrophysics

151

Pulsars, Supernova Remnants, X Ray Sources, Nebulae, Periodic Variations

Scientific paper

A pulsing X-ray source has been discovered within the shell of the supernova remnant MSH 15-52. The period is 0.150 s, and the rate of increase of period with time is the highest measured for any pulsar. These characteristics and the fact that the pulsar is surrounded by a small, bright nebula indicate that this object is very similar to the Crab pulsar.

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