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

1996/09/26 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/9609185

8 pages and one PostScript figure. Presented as a poster on the NATO ASI "The many faces of neutron stars", Lipari, October 1-10, 1996

arxiv created 1996/09/26 · arxiv updated 2009/12/01

Abstract

In 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).

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• Spin evolution of neutron stars
• Spin and magnetism in old neutron stars
• Stochastic spin evolution of neutron stars
• Growth of the Magnetic Field in Young Neutron Stars
• X-ray observations of Isolated Neutron Stars