Explanations of pulsar velocities

Astronomy and Astrophysics – Astrophysics

Scientific paper

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7 pages, revtex, epsf, two figures included, talk presented at APS Division of Particles and Fields Conference (DPF'99), UCLA,

Scientific paper

Several mechanisms based on neutrino oscillations can explain the observed
motions of pulsars if the magnetic field in their interiors is of order
10^{14}-10^{15} G.

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