The Binary History and the Magnetic Field of Neutron Stars

dc.contributor.author	Konar, S
dc.date.accessioned	2008-05-27T12:06:42Z
dc.date.available	2008-05-27T12:06:42Z
dc.date.issued	2003
dc.identifier.citation	BASI, Vol. 31, No. 3&4, pp. 187 - 193	en
dc.identifier.uri	http://hdl.handle.net/2248/2363
dc.description.abstract	There has been strong observational evidence suggesting a casual connection between the binary history of neutron stars and the evolution of their magnetic field. In this article we discuss one of 3 the plausible mechanisms proposed for the evolution of the surface magnetic field, that of the diamagnetic screening of the field by accreted material.	en
dc.format.extent	224124 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.relation.uri	http://adsabs.harvard.edu/abs/2003BASI...31..187K	en
dc.subject	Magnetic fields	en
dc.subject	Neutron stars	en
dc.subject	Accretion-material flow	en
dc.title	The Binary History and the Magnetic Field of Neutron Stars	en
dc.type	Article	en