SIMBAD references

2012ApJ...761...66S - Astrophys. J., 761, 66 (2012/December-2)

Post-outburst X-ray flux and timing evolution of Swift J1822.3-1606.

SCHOLZ P., NG C.-Y., LIVINGSTONE M.A., KASPI V.M., CUMMING A. and ARCHIBALD R.F.

Abstract (from CDS):

Swift J1822.3-1606 was discovered on 2011 July 14 by the Swift Burst Alert Telescope following the detection of several bursts. The source was found to have a period of 8.4377 s and was identified as a magnetar. Here we present a phase-connected timing analysis and the evolution of the flux and spectral properties using Rossi X-ray Timing Explorer, Swift, and Chandra observations. We measure a spin frequency of 0.1185154343(8)/s and a frequency derivative of -4.3±0.3x10–15 at MJD 55761.0, in a timing analysis that includes significant non-zero second and third frequency derivatives that we attribute to timing noise. This corresponds to an estimated spin-down inferred dipole magnetic field of B ∼ 5x1013 G, consistent with previous estimates though still possibly affected by unmodeled noise. We find that the post-outburst 1-10 keV flux evolution can be characterized by a double-exponential decay with decay timescales of 15.5±0.5 and 177±14 days. We also fit the light curve with a crustal cooling model, which suggests that the cooling results from heat injection into the outer crust. We find that the hardness-flux correlation observed in magnetar outbursts also characterizes the outburst of Swift J1822.3-1606. We compare the properties of Swift J1822.3-1606 with those of other magnetars and their outbursts.

Abstract Copyright:

Journal keyword(s): pulsars: individual: Swift J1822.3-1606 - stars: neutron - X-rays: bursts - X-rays: general

Simbad objects: 11

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2021.03.04-10:42:54

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