Unveiling the broad band properties of the fading transient AXP XTE J1810-197

Details Unveiling the broad band properties of the fading transient AXP XTE J1810-197 Unveiling the broad band properties of the fading transient AXP XTE J1810-197

Oct 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005xmm..prop..248i&link_type=abstract

XMM-Newton Proposal ID #04068002

Computer Science

Supernovae, Supernova Remnants, Diffuse (Galactic) Emission And Isolated Neutron Stars, Xte J1810-197, Xte J1810-197, Xmm-Newton Proposal 04068002

Scientific paper

This XMM program is aimed at continuing the monitoring the fading phases of the Anomalous X-ray Pulsar (AXP), XTE J1810-197. The transient behaviour of this source, unique amongst AXPs, will make it possible to study its properties over an unprecedented range of flux levels and energies. This source might thus represent a ``Rosetta stone'' for our understanding of the nature and emission mechanism of AXPs, and of a unified scheme for isolated neutron stars (NSs) encompassing apparently dissimilar classes, such as radio pulsars, dim NSs and central compact objects (CCOs) in supernova remnants.

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