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Paper detail

Modelling lightcurves and spectra of transient Anomalous X-ray Pulsars

We present the first detailed joint modelling of both the timing and spectral properties during the outburst decay of transient anomalous X-ray pulsars. We consider the two sources XTE J1810-197 and CXOU J164710.2-455216, and describe the source decline in the framework of a twisted magnetosphere model, using Monte Carlo simulations of magnetospheric scattering and mimicking localized heat deposition at the NS surface following the activity. Our results support a picture in which a limited portion of the star surface close to one of the magnetic poles is heated at the outburst onset. The subsequent evolution is driven both by the cooling/varying size of the heated cap and by a progressive untwisting of the magnetosphere.

preprint2011arXivOpen access
S. ZaneA. AlbanoR. TurollaG. L. IsraelL. NobiliL. Stella
astro-ph.HE
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S. ZaneA. AlbanoR. TurollaG. L. IsraelL. NobiliL. Stella

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