Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/1577
Title: Magnetic field evolution of accreting neutron stars - III
Authors: Konar, Sushan
Bhattacharya, D.
Issue Date: Sep-1999
Publisher: Blackwell Scientific for the Royal Astronomical Society
Citation: Monthly Notices of the Royal Astronomical Society, 1999, Vol.308, p795-798.
Abstract: The evolutionary scenario of a neutron star magnetic field is examined assuming a spin-down induced expulsion of magnetic flux originally confined to the core, in a case in which the expelled flux undergoes ohmic decay. The nature of field evolution, for accreting neutron stars, is investigated incorporating the crustal microphysics and material movement resulting from accretion. This scenario may explain the observed field strengths of neutron stars but only if the crustal lattice contains a large amount of impurity, which is in direct contrast to the models that assume an original crustal field.
Description: Open Access
URI: http://hdl.handle.net/2289/1577
ISSN: 0004-6361
Alternative Location: http://adsabs.harvard.edu/cgi-bin/bib_query?1999MNRAS.308..795K
http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999MNRAS.308..795K&link_type=ARTICLE&db_key=AST
Copyright: (1999) Royal Astronomical Society
Appears in Collections:Research Papers (A&A)

Files in This Item:
File Description SizeFormat 
1999_MNRAS_Vol.308_p795.pdfOpen Access213.45 kBAdobe PDFView/Open


Items in RRI Digital Repository are protected by copyright, with all rights reserved, unless otherwise indicated.