SIMBAD references

2011ApJ...732L...4A - Astrophys. J., 732, L4 (2011/May-1)

SGR 0418+5729–How does a young neutron star spin down to a 9 s period with a dipole field less than 1013 g?

ALPAR M.A., ERTAN U. and CALISKAN S.

Abstract (from CDS):

The period derivative bound for the soft gamma-ray repeater SGR 0418+5729 establishes the magnetic dipole moment to be distinctly lower than the magnetar range, placing the source beyond the regime of isolated pulsar activity in the P-{dot}P diagram and giving a characteristic age >2x107 yr, much older than the 105 yr age range of SGRs and anomalous X-ray pulsars. So the spin-down must be produced by a mechanism other than dipole radiation in vacuum. A fallback disk will spin down a neutron star with surface dipole magnetic field in the 1012 G range and initial rotation period P0∼ 100 ms to the 9.1 s period of SGR 0418+5729 in a few 104 to ∼105 yr. The current upper limit to the period derivative gives a lower limit of ∼105 yr to the age that is not sensitive to the neutron star's initial conditions. The total magnetic field on the surface of SGR 0418+5729 could be significantly larger than its 1012 G dipole component.

Abstract Copyright: ∼

Journal keyword(s): accretion, accretion disks - pulsars: individual: AXPs - stars: neutron - X-rays: bursts

Simbad objects: 5

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