Magnetic fields of neutron stars in X-ray pulsars
Astrophysics
2007-05-23 v1
Abstract
Estimates of the magnetic field of neutron stars in X-ray pulsars are obtained using the hypothesis of the equilibrium period for disk and wind accretion and also from the BATSE data on timing of X-ray pulsars using the observed maximum spin-down rate. Cyclotron lines at energies keV in several Be-transient are predicted for future observations.
Cite
@article{arxiv.astro-ph/9908234,
title = {Magnetic fields of neutron stars in X-ray pulsars},
author = {V. M. Lipunov and S. B. Popov},
journal= {arXiv preprint arXiv:astro-ph/9908234},
year = {2007}
}
Comments
9 pages, 4 PostScript figures, 3 tables