2013MNRAS.428.1438C

Query : 2013MNRAS.428.1438C

2013MNRAS.428.1438C - Mon. Not. R. Astron. Soc., 428, 1438-1441 (2013/January-2)

Growth of magnetic fields in accreting millisecond pulsars.

CUOFANO C., DRAGO A. and PAGLIARA G.

Abstract (from CDS):

R-modes can generate strong magnetic fields in the core of accreting millisecond neutron stars. The diffusion of these fields outside the core causes the growth of the external magnetic field and thus it affects the evolution of the spin-down rates {dot}P of the millisecond pulsars (MSPs). The diffusion of the internal magnetic field provides a new evolutionary path for the MSPs. This scenario could explain the large {dot}P of the pulsars J1823-3021A and J1824-2452A.

Abstract Copyright: © 2012 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society (2012)

Journal keyword(s): stars: magnetic field - stars: neutron - stars: low-mass - pulsars: general - pulsars: individual: J1823-3021A - pulsars: individual: J1824-2452A

Simbad objects: 4

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Number of rows : 4
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 J1820-30A Psr 18 23 40.4842 -30 21 39.920           ~ 168 1
2 NGC 6624 GlC 18 23 40.51 -30 21 39.7           ~ 939 1
3 PSR J1824-2452A Psr 18 24 32.009 -24 52 11.10           ~ 529 2
4 M 28 GlC 18 24 32.89 -24 52 11.4           ~ 821 0

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