Please use this identifier to cite or link to this item:
|Title:||Magnetic field evolution of accreting neutron stars - III|
|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:||Sorry, the full-text is not available here. Please click on the alternative location to access it.|
|Copyright:||(1999) Royal Astronomical Society|
|Appears in Collections:||Research Papers (A&A)|
Files in This Item:
There are no files associated with this item.
Items in RRI Digital Repository are protected by copyright, with all rights reserved, unless otherwise indicated.