Magnetic fields of neutron stars in X-ray pulsars

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dc.creatorLipunov, V. M.
dc.creatorPopov, S. B.
dc.date1999-08-20
dc.date.accessioned2026-07-07T02:32:53Z
dc.date.available2026-07-07T02:32:53Z
dc.descriptionEstimates 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.
dc.description9 pages, 4 PostScript figures, 3 tables
dc.identifierhttps://arxiv.org/abs/astro-ph/9908234
dc.identifierhttp://arxiv.org/abs/astro-ph/9908234
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/14623
dc.subjectAstrophysics
dc.titleMagnetic fields of neutron stars in X-ray pulsars
dc.typetext

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