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Disk-assisted Spin-down of Young Radio Pulsars

ASTROPHYSICAL JOURNAL, no. 1 (2001): L63-L66

Cited by: 79|Views5

Abstract

We present a model for the spin-down of young radio pulsars in which the neutron star loses rotational energy not only by emitting magnetic dipole radiation but also by torquing a surrounding disk produced by supernova fallback. The braking index predicted in our model is, in general, less than n = 3 (the value for pure magnetic dipole ra...More

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