Spin and its evolution for isolated neutron stars and X-ray binaries: the determination of the 'Diffusion coefficients' and Spindown Theorem
arXiv:astro-ph/9609185
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).
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