Magnetic fields in neutron stars, white dwarfs and implications for binary millisecond pulsars
In this paper, we show that the range in magnetic fluxes that is observed in the chemically peculiar Ap, Bp and Op stars is similar to that measured in the High Field Magnetic White Dwarfs and the Neutron Stars, which suggests that the magnetic flux is approximately conserved during stellar evolution at least for intermediate to high mass stars. We also discuss the recent evidence of a bi-modal distribution of magnetic fields in white dwarfs and its implications for the accretion induced collapse hypothesis for the origin of the binary millisecond pulsars.
Neutron stars pulsars white dwarfs magnetic fields
Lilia Ferrario D. T. Wickramasinghe
Department of Mathematics, Mathematical Sciences Institute, The Australian National University, ACT 0200, Australia
国际会议
紧凑型物体的天体物理学国际会议(International Conference on Astrophysics of Compact Objects)
安徽黄山
英文
188-193
2007-07-01（万方平台首次上网日期，不代表论文的发表时间）