1999/08/20 by V. M. Lipunov, Lipunov, V. M., S. B. Popov +1
Physics and Astronomy · #Astrophysics (astro-ph) #FOS: Physical sciences #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/9908234
9 pages, 4 PostScript figures, 3 tables
arxiv created 1999/08/20 · arxiv updated 2009/12/01
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 ≥ 100 keV in several Be-transient are predicted for future observations.