Spin and its evolution for isolated neutron stars and X-ray binaries: the determination of the 'Diffusion coefficients' and Spindown Theorem

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dc.creatorLipunov, V. M.
dc.creatorPopov, S. B.
dc.date1996-09-26
dc.date.accessioned2026-07-07T02:21:58Z
dc.date.available2026-07-07T02:21:58Z
dc.descriptionIn this work we give detail consideration of the possible scenario of evolution of isolated neutron stars and determine some characteristics of X-ray pulsars from their spin period evolution (the paper containes more detailed abstract).
dc.description8 pages and one PostScript figure. Presented as a poster on the NATO ASI "The many faces of neutron stars", Lipari, October 1-10, 1996
dc.identifierhttps://arxiv.org/abs/astro-ph/9609185
dc.identifierhttp://arxiv.org/abs/astro-ph/9609185
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/10704
dc.subjectAstrophysics
dc.titleSpin and its evolution for isolated neutron stars and X-ray binaries: the determination of the 'Diffusion coefficients' and Spindown Theorem
dc.typetext

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