2002MNRAS.335..733J


Query : 2002MNRAS.335..733J

2002MNRAS.335..733J - Mon. Not. R. Astron. Soc., 335, 733-740 (2002/September-3)

Post-glitch relaxation in pulsars.

JONES P.B.

Abstract (from CDS):

The glitch model of Ruderman, Zhu & Chen is applied to the problem of post-glitch relaxation. The energy dissipated in a glitch is such that motion of both solid and liquid phases during and after spin-up is strictly constrained to surfaces of constant chemical composition. The amorphous and heterogeneous nature of the solid phase of neutron star matter is used to deduce the qualitative form of the dissipative force acting on unit length of a neutron vortex as a function of its velocity. The analysis of post-glitch relaxation given here is necessarily qualitative owing to the stochastic nature of the model, but is consistent with both the normal and anomalous cases observed.

Abstract Copyright: RAS

Journal keyword(s): stars: neutron - pulsars: general.

Simbad objects: 8

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Number of rows : 8
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 NAME Vela Pulsar Psr 08 35 20.65525 -45 10 35.1545     15.10     ~ 2446 1
2 PSR B1046-58 Psr 10 48 13.10000 -58 32 03.0000           ~ 293 0
3 PSR B1240-64 Psr 12 43 17.2912183824 -64 23 23.082548820           ~ 119 0
4 PSR B1338-62 Psr 13 41 42.63 -62 20 20.7           ~ 152 1
5 PSR B1641-45 Psr 16 44 49.28482 -45 59 09.6360     12.60     ~ 217 0
6 PSR B1737-30.2 Psr 17 40 33.98000 -30 15 22.0000           ~ 236 0
7 PSR B1757-24 Psr 18 01 00.016 -24 51 27.50           ~ 258 1
8 PSR B1822-09 Psr 18 25 30.62000 -09 35 22.0000           ~ 382 0

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