Supernova SN 1987A - Rotation rate of the central pulsar

Details Supernova SN 1987A - Rotation rate of the central pulsar Supernova SN 1987A - Rotation rate of the central pulsar

Apr 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989mnras.237.1033b&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 237, April 15, 1989, p. 1033-1036.

Astronomy and Astrophysics

Astronomy

Pulsars, Stellar Rotation, Supernova 1987A, Light Curve, Stellar Luminosity, Stellar Magnetic Fields, Stellar Mass Accretion

Scientific paper

Using available observational data on supernova SN 1987A, firm
quantitative lower limits on the rotation period of the central pulsar
(assuming the pulsar luminosity to power the supernova light curve) are
derived. It is also demonstrated that pulsars born in type II supernovae
are, in general, unlikely to be fast pulsars.

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