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- W2009688085 abstract "It is shown that, when angular-momentum losses of a radio pulsar are represented as a sum of magnetic-dipole and current losses, the angle between the magnetic moment and rotation axis of the radio pulsar tends to some equilibrium value (near 45°). This process takes place on a timescale of the order of the pulsar’s characteristic age. Taking into account the non-dipolarity of the pulsar’s magnetic field changes this equilibrium angle." @default.
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- W2009688085 date "2009-12-01" @default.
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- W2009688085 title "Evolution of the angle between the magnetic moment and the rotation axis of radio pulsars" @default.
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- W2009688085 doi "https://doi.org/10.1134/s1063772909120075" @default.
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