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The Ecology of Magnetic Rotators

Published online by Cambridge University Press:  25 May 2016

V.M. Lipunov*
Affiliation:
Sternberg Astronomical Institute, Universitetskij pr. 13, 119899, Moscow V-234, Russia

Abstract

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A review is given concerning the current state of the theory of evolution of magnetic compact stars. The intrinsic evolution of the magnetized compact star is shown, both theoretically and numerically, to be the decisive factor in explaining observable properties, and in predicting yet unknown properties of high-energy radiation sources in our and other galaxies. The main results are given of recent evolutionary scenario simulations (Scenario Machine) by the Monte-Carlo method.

Type
1 Binary Evolution
Copyright
Copyright © Kluwer 1996 

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