Astronomy and Astrophysics – Astrophysics – High Energy Astrophysical Phenomena
Scientific paper
2010-12-07
ApJ 728, 75 (2011)
Astronomy and Astrophysics
Astrophysics
High Energy Astrophysical Phenomena
10 pages, 3 color figures
Scientific paper
10.1088/0004-637X/728/2/75
We examine the recoil velocity induced by the superposition of the magnetic dipole and quadrupole radiation from a pulsar/magnetar born with rapid rotation. The resultant velocity depends on not the magnitude, but rather the ratio of the two moments and their geometrical configuration. The model does not necessarily lead to high spatial velocity for a magnetar with a strong magnetic field, which is consistent with the recent observational upper bound. The maximum velocity predicted with this model is slightly smaller than that of observed fast-moving pulsars.
Kato Yugo E.
Kojima Yasufumi
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