@inproceedings{a9da500e3f3640f5b81c333c17d73cb9,
title = "Numerical simulations of magnetorotational supernovae",
abstract = "We carry out series of numerical simulations on the magnetorotational supernovae in order to study about recoil of so-called {"}magnetars{"}, highly magnetized slowly rotating neutron stars. We assume that the core initially rotates rapidly and is strongly magnetized. Presumed initial magnetic fields have dipole-like configurations somewhat offset from the center of the cores. As a result, equatorially asymmetric supernova explosions are produced and recoil velocities of ∼500-1000kms-1 are obtained which suggest that magnetars possibly have large recoil velocities as ordinary pulsars.",
keywords = "MHD, Magnetars, Numerical simulations, Proper motions, Supernovae",
author = "Hidetomo Sawai and Kei Kotake and Shoichi Yamada",
year = "2007",
doi = "10.1063/1.2803577",
language = "English",
isbn = "0735404488",
series = "AIP Conference Proceedings",
pages = "280--283",
booktitle = "SUPERNOVA 1987A",
note = "SUPERNOVA 1987A: 20 YEARS AFTER: Supernovae and Gamma-Ray Bursters ; Conference date: 19-02-2007 Through 23-02-2007",
}