Diamagnetic screening of the magnetic field in accreting neutron stars

dc.contributor.author	Konar, S
dc.contributor.author	Choudhuri, A. R
dc.date.accessioned	2008-07-22T07:53:08Z
dc.date.available	2008-07-22T07:53:08Z
dc.date.issued	2002-09
dc.identifier.citation	BASI, Vol. 30, No. 3, pp. 697 - 698	en
dc.identifier.uri	http://hdl.handle.net/2248/2795
dc.description.abstract	A possible mechanism for screening of the surface magnetic field of an accreting neutron star, by the accreted material, is investigated. In particular, we investigate the nature of the evolution of the internal field configuration in the case of a) a polar cap accretion and b) spherical accretion.	en
dc.format.extent	81195 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.subject	Magnetic Fields	en
dc.subject	Neutron Stars	en
dc.subject	Accretion-Material Flow	en
dc.title	Diamagnetic screening of the magnetic field in accreting neutron stars	en
dc.type	Article	en