2015MNRAS.451.2564G

Query : 2015MNRAS.451.2564G

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

goto Full paper

goto View the references in ADS

Number of rows : 2
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026 		#notes
1 PSR J1210-5226 Psr 12 10 00.88 -52 26 28.4           ~ 230 1
2 PSR J1824-2452A Psr 18 24 32.009 -24 52 11.10           ~ 529 2

To bookmark this query, right click on this link: simbad:objects in 2015MNRAS.451.2564G and select 'bookmark this link' or equivalent in the popup menu