A New Magnetar in a Young Supernova Remnant

Details A New Magnetar in a Young Supernova Remnant A New Magnetar in a Young Supernova Remnant

Oct 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005xmm..prop..113g&link_type=abstract

XMM-Newton Proposal ID #04029101

Other

Supernovae, Supernova Remnants, Diffuse (Galactic) Emission And Isolated Neutron Stars, 1E 1547.0-5408, Xmm-Newton Proposal 04029101

Scientific paper

Anomalous X-ray Pulsars (AXPs) are an exotic population of pulsating X-ray sources, which are now thought to be highly magnetized neutron stars ("magnetars"). However, the evolution, demography, and relation of magnetars to other types of neutron star are all not yet understood. We have identified a new candidate association between an AXP and a young supernova remnant (SNR), for which we propose XMM and Chandra observations. These data can confirm our AXP and SNR identifications, and can thus help constrain the origin, evolution and physical properties of the magnetar population.

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