Monitoring the transient AXP 1E1547.0-5408: from outburst to quiescence

Details Monitoring the transient AXP 1E1547.0-5408: from outburst to quiescence Monitoring the transient AXP 1E1547.0-5408: from outburst to quiescence

Oct 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009xmm..prop..193b&link_type=abstract

XMM-Newton Proposal ID #06557301

Physics

Supernovae, Supernova Remnants, Diffuse (Galactic) Emission And Isolated Neutron Stars, Axp 1E 1547.0-5

Scientific paper

This program is aimed at continuing the successful monitoring of the fading phases of the transient Anomalous X-ray Pulsar 1E1547.0-5408 following its Jan 2009 outburst. The peculiar X-ray behaviour of this source, the only one among AXPs that showed two different outbursts, allowed to study its properties over an unprecedented range of fluxes and to get valuable information on the yet debated processes governing the outburst onset and its log term evolution. The last pointing we are requesting is aimed at continuing the study of the outburst properties, as the source approaches the quiescent state, and checking the presence of permanent spectral/timing changes induced by the outburst, if any.

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