Computer Science
Scientific paper
Oct 2004
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004xmm..prop...43g&link_type=abstract
XMM-Newton Proposal ID #03012701
Computer Science
Supernovae, Supernova Remnants, Diffuse (Galactic) Emission And Isolated Neutron Stars, Cxou J180951.0-, Xmm-Newton Proposal 03012701
Scientific paper
The recently discovered 5.5s pulsar XTE J1810-197 is the first confirmed Transient Anomalous X-ray Pulsar (TAXP), likely a magnetar with a huge magnetic field of 3E14 G. XTE J1810-197 is currently in outburst but fading with a 300 day e-fold time. Archival data spanning 24 yrs indicate that this is a short-lived active state, which implies the existence of a vast population of unexplored young NSs. From its lack of pulsations and softer spectrum in quiescence, XTE J1810-197 may also hold the key to unify the magnetar model for SGRs, AXPs, and central compact objects in SNRs. We propose to continue our semi-annual XMM monitoring campaign of XTE J1810-197 to follow its flux, spin, and spectral evolution, to capture for the first time a complete cycle of a TAXP from quiescence, to outburst, and back.
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