Query : 2006A&A...451.1049B

2006A&A...451.1049B - Astronomy and Astrophysics, volume 451, 1049-1052 (2006/6-1)

Protoneutron star dynamos: pulsars, magnetars, and radio-silent X-ray emitting neutron stars.


Abstract (from CDS):

We discuss the mean-field dynamo action in protoneutron stars that are subject to instabilities during the early evolutionary phase. The mean field is generated in the neutron-finger unstable region where the Rossby number is ∼1 and mean-field dynamo is efficient. Depending on the rotation rate, the mean-field dynamo can lead to the formation of three different types of pulsars. If the initial period of the protoneutron star is short, then the generated large-scale field is very strong (>3x1013G) and exceeds the small-scale field at the neutron star surface. If rotation is moderate, then the pulsars are formed with more or less standard dipole fields (<3x1013G) but with surface small-scale magnetic fields stronger than the dipole field. If rotation is very slow, then the mean-field dynamo does not operate, and the neutron star has no global field. Nevertheless, strong small-scale fields are generated in such pulsars, and they can manifest themselves as objects with very low spin-down rate but with a strong magnetic field inferred from the spectral features.

Abstract Copyright:

Journal keyword(s): magnetohydrodynamics (MHD) - pulsars: general - stars: neutron - X-ray: stars - stars: magnetic fields

Simbad objects: 5

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Number of rows : 5
N Identifier Otype ICRS (J2000)
ICRS (J2000)
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2022
1 PSR B0154+61 Psr 01 57 49.930 +62 12 25.90           ~ 115 0
2 PSR J1119-6127 Psr 11 19 14.30 -61 27 49.5           ~ 369 1
3 PSR J1718-3718 Psr 17 18 10.16 -37 18 53.8           ~ 68 0
4 PSR B1811-17.7 Psr 18 14 43.10 -17 44 48.0           ~ 72 0
5 PSR J1847-0130 Psr 18 47 35.2 -01 30 46           ~ 42 0

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