SIMBAD references

2015MNRAS.451.2564G - Mon. Not. R. Astron. Soc., 451, 2564-2574 (2015/August-2)

Magnetic field inertia and rotation dynamics of radio pulsars.

GOGLICHIDZE O.A., BARSUKOV D.P. and TSYGAN A.I.

Abstract (from CDS):

In this article, we discuss the magnetic field inertia that results in the so-called anomalous electromagnetic torque, making neutron stars precess. We focus particularly on the relative contribution of fields of different scales and show that small-scale fields may produce an anomalous torque comparable in magnitude with the one produced by dipolar field. Also, the internal toroidal field may play an important role. If the stellar magnetic field is not symmetric with respect to the dipolar moment axis, the pulsar inclination angle may oscillate with a typical amplitude of tens of degrees, due to precession. Such variations may, in principle, be observable.

Abstract Copyright: © 2015 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society (2015)

Journal keyword(s): stars: magnetic field - stars: neutron - pulsars: general

CDS comments: In Introduction : PSR B1821+24 is a misprint for PSR B1821-24.

Simbad objects: 2

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