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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3640
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dc.contributor.authorBhatt, H. C-
dc.contributor.authorDatta, B-
dc.date.accessioned2008-09-16T14:05:42Z-
dc.date.available2008-09-16T14:05:42Z-
dc.date.issued1989-04-
dc.identifier.citationMonthly Notices of the Royal Astronomical Society, Vol. 237, pp. 1033 - 1036en
dc.identifier.issn0035-8711-
dc.identifier.urihttp://hdl.handle.net/2248/3640-
dc.description.abstractUsing 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.en
dc.publisherRoyal Astronomical Societyen
dc.relation.urihttp://ads.iucaa.ernet.in/abs/1989MNRAS.237.1033Ben
dc.subjectPulsarsen
dc.subjectStellar Rotationen
dc.subjectSupernova 1987aen
dc.subjectLight Curveen
dc.subjectStellar Luminosityen
dc.subjectStellar Magnetic Fieldsen
dc.subjectStellar Mass Accretionen
dc.titleSupernova SN 1987A - Rotation rate of the central pulsaren
dc.typeArticleen
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