The Anatomy of a Magnetar: XMM Monitoring of the Transient Anomalous X-ray Pulsar XTE J1810-197

dc.creatorGotthelf, E. V.
dc.creatorHalpern, J. P.
dc.date2006-08-22
dc.date.accessioned2026-07-07T10:39:50Z
dc.date.available2026-07-07T10:39:50Z
dc.descriptionWe present the latest results from a multi-epoch timing and spectral study of the Transient Anomalous X-ray Pulsar XTE J1810-197. We have acquired seven observations of this pulsar with the Newton X-ray Multi-mirror Mission (XMM-Newton) over the course of two and a half years, to follow the spectral evolution as the source fades from outburst. The spectrum is arguably best characterized by a two-temperature blackbody whose luminosities are decreasing exponentially with tau_1 = 870 days and tau_2 = 280 days, respectively. The temperatures of these components are currently cooling at a rate of 22% per year from a nearly constant value recorded at earlier epochs of kT_1 = 0.25 keV and kT_2 = 0.67 keV, respectively. The new data show that the temperature T_1 and luminosity of that component have nearly returned to their historic quiescent levels and that its pulsed fraction, which has steadily decreased with time, is now consistent with the previous lack of detected pulsations in quiescence. We also summarize the detections of radio emission from XTE J1810-197, the first confirmed for any AXP. We consider possible models for the emission geometry and mechanisms of XTE J1810-197.
dc.description8 pages, 7 figures, 1 table, latex. To appear in the proceedings of "Isolated Neutron Stars", Astrophysics & Space Science, in press
dc.identifierhttps://arxiv.org/abs/astro-ph/0608473
dc.identifierhttp://arxiv.org/abs/astro-ph/0608473
dc.identifierAstrophys.SpaceSci.308:79-87,2007
dc.identifierdoi:10.1007/s10509-007-9327-9
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/181169
dc.subjectAstrophysics
dc.titleThe Anatomy of a Magnetar: XMM Monitoring of the Transient Anomalous X-ray Pulsar XTE J1810-197
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