Recoils of Magnetars

Computer Science

Scientific paper

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Neutron Stars

Scientific paper

We study the recoil of so-called ``magnetars'', highly magnetized slowly rotating neutron stars, doing series of numerical simulations on the core-collapse of massive stars in strong magnetic field and rapid rotation regime. We assume that the initial magnetic fields have a dipole-like configurations somewhat offset from the center of the cores. As a result, recoil velocities of ~ 500 - 1000 km s-1 are obtained which suggest that magnetars could have substantial recoil velocities as ordinary pulsars.

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