On the implications of the radio and X-ray pulsar in the supernova remnant MSH 15-52

Details On the implications of the radio and X-ray pulsar in the supernova remnant MSH 15-52 On the implications of the radio and X-ray pulsar in the supernova remnant MSH 15-52

Jun 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982csci...51..596s&link_type=abstract

Current Science, Vol. 51, pp. 596-599 (1982)

Computer Science

8

Scientific paper

Comparison of the X-ray nebulosity surrounding the X-ray and radio
pulsar in the shell-type SNR MSH 15-52 with the Crab nebula leads to an
initial period for the pulsar ~70 ms. The association of the pulsar with
the shell remnant confirms the validity of the Σ-t approach in
determining the ages of young SNRs using historical calibrators.

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