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Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/1582
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dc.contributor.authorKonar, Sushan-
dc.contributor.authorBhattacharya, D.-
dc.date.accessioned2006-12-14T07:43:20Z-
dc.date.available2006-12-14T07:43:20Z-
dc.date.issued1999-03-
dc.identifier.citationMonthly Notices of the Royal Astronomical Society, 1999, Vol.303, p588-594en
dc.identifier.issn0004-6361-
dc.identifier.urihttp://hdl.handle.net/2289/1582-
dc.descriptionOpen Accessen
dc.description.abstractWe investigate the evolution of the magnetic fields of isolated pulsars and neutron stars in different kinds of binary systems, assuming the field to be originally confined to the crust. Our results for the field evolution in isolated neutron stars help us to constrain the physical parameters of the crust. By modelling the full evolution of a neutron star in a binary system through several stages of interaction, we can compare the resulting final field strength with that observed in neutron stars in various types of binary systems. One of the interesting aspects of our results is a positive correlation between the rate of accretion and the final field strength, for which some observational indication already exists. Our results also match the overall picture of the field evolution in neutron stars derived from observations.en
dc.format.extent8338 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherBlackwell Publishing for the Royal Astronomical Societyen
dc.relation.urihttp://adsabs.harvard.edu/cgi-bin/bib_query?1999MNRAS.303..588Ken
dc.relation.urihttp://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999MNRAS.303..588K&link_type=ARTICLE&db_key=ASTen
dc.rights(1999) Royal Astronomical Societyen
dc.subjectMagnetic fieldsen
dc.subjectBinariesen
dc.subjectStars:magnetic fieldsen
dc.subjectNeutron starsen
dc.subjectPulsarsen
dc.titleMagnetic field evolution of accreting neutron stars - IIen
dc.typeArticleen
Appears in Collections:Research Papers (A&A)

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