Evolution of the multipolar magnetic field in isolated neutron stars

Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/1569

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DC Field	Value	Language
dc.contributor.author	Mitra, D.	-
dc.contributor.author	Konar, Sushan	-
dc.contributor.author	Bhattacharya, D.	-
dc.date.accessioned	2006-12-13T07:30:29Z	-
dc.date.available	2006-12-13T07:30:29Z	-
dc.date.issued	1999-08	-
dc.identifier.citation	Monthly Notices of the Royal Astronomical Society, 1999, Vol.307, p459 -462	en
dc.identifier.issn	0004-6361	-
dc.identifier.uri	http://hdl.handle.net/2289/1569	-
dc.description	Open Access	-
dc.description.abstract	The evolution of the multipolar structure of the magnetic field of isolated neutron stars is studied assuming the currents to be confined to the crust. We find that, except for multipoles of very high order (l〉~25), the evolution is similar to that of a dipole. Therefore no significant evolution is expected in the pulse shape of isolated radio pulsars because of the evolution of the multipole structure of the magnetic field.	en
dc.format.extent	8338 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Springer-Verlag	en
dc.relation.uri	http://adsabs.harvard.edu/cgi-bin/bib_query?1999MNRAS.307..459M	en
dc.relation.uri	http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999MNRAS.307..459M&link_type=ARTICLE&db_key=AST	en
dc.rights	(1999) by the Royal Astronomical Society	en
dc.title	Evolution of the multipolar magnetic field in isolated neutron stars	en
dc.type	Article	en
Appears in Collections:	Research Papers (A&A)

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