Magnetic fields of neutron stars in X-ray pulsars

Details Magnetic fields of neutron stars in X-ray pulsars Magnetic fields of neutron stars in X-ray pulsars

1999-08-20

arxiv.org/abs/astro-ph/9908234v1

Astronomy and Astrophysics

Astrophysics

9 pages, 4 PostScript figures, 3 tables

Scientific paper

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 $\ge 100$ keV in
several Be-transient are predicted for future observations.

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