2010MNRAS.409.1077B


Query : 2010MNRAS.409.1077B

2010MNRAS.409.1077B - Mon. Not. R. Astron. Soc., 409, 1077-1087 (2010/December-2)

The influence of nondipolar magnetic field and neutron star precession on braking indices of radiopulsars.

BARSUKOV D.P. and TSYGAN A.I.

Abstract (from CDS):

Some radiopulsars have anomalous braking index values {img}. It is shown that such anomalous values may be related to nondipolar magnetic field. Precession of a neutron star leads to rotation (in the reference frame of the star) of its angular velocity Ω around the direction of neutron star magnetic dipole m with an angular velocity Ωp. This process may cause altering of electric current flowing through the inner gap and consequently the current losses on the time-scale of precession period Tp= 2π/Ωp. It occurs because the electric current in the inner gap is determined by Goldreich-Julian charge density ρGJ=-Ω⋅B/(2πc), that depends on the angle between direction of small scale magnetic field and the angular velocity Ω.

Abstract Copyright: 2010 The Authors. Journal compilation2010 RAS

Journal keyword(s): stars: pulsar: general - stars: neutron

Simbad objects: 7

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Number of rows : 7
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 M 1 SNR 05 34 31.8 +22 01 03           ~ 6516 1
2 V* CM Tau Psr 05 34 31.9474694616 +22 00 52.153698024           ~ 5476 0
3 PSR B0656+14 Psr 06 59 48.18800 +14 14 19.2000   24.85 24.90     ~ 943 1
4 NAME Vela Pulsar Psr 08 35 20.65525 -45 10 35.1545     15.10     ~ 2446 1
5 PSR B1719-37 Psr 17 22 59.17000 -37 12 03.0000           ~ 107 0
6 PSR B1915+13 Psr 19 17 39.79400 +13 53 57.1600           ~ 190 0
7 PSR B2000+32 Psr 20 02 04.424 +32 17 18.31           ~ 51 0

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