Physics
Scientific paper
Oct 2007
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007xmm..prop..163i&link_type=abstract
XMM-Newton Proposal ID #05553502
Physics
Supernovae, Supernova Remnants, Diffuse (Galactic) Emission And Isolated Neutron Stars, Cxo J164710.2-4, Cxo J164710.2-4, Xmm-Newton Proposal Id #05553502
Scientific paper
On September 2006 an intense (10^39 ergs) and short (20ms) burst was detected by Swift from the candidate Anomalous X-ray Pulsar CXOU J164710.2-455216. A Swift observations carried out 13 hours later found that the AXP entered in a rare outburst phase and measured a flux level 300 times brighter then that in quiescence. Subsequent Swift, Chandra, XMM and SUZAKU follow-up observations monitored the initial phases of the source outburst allowing to infer very important information for this source. Both the spectral and timing properties of CXOU J164710.2-455216 drastically changed and are still evolving after one year. The present proposal is aimed at following the evolution of the main spectral/timing parameters of the second confirmed bursting transient AXP.
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