Some conclusions on the magnetic fields of neutron stars in atoll and Z sources

Abstract

The main conclusions of the accretion induced neutron star magnetic field evolution model are described, and it is found that a bright Z source possesses a stronger field than that of on Atoll source and local strong field may exist in the recycled neutron stars or millisecond pulsars on account of the field line distribution. © 2008 Springer-Verlag Berlin Heidelberg.