Completing the X-ray census of Plerionic Supernova Remnants within 7 kpc

Details Completing the X-ray census of Plerionic Supernova Remnants within 7 kpc Completing the X-ray census of Plerionic Supernova Remnants within 7 kpc

Oct 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005xmm..prop...36k&link_type=abstract

XMM-Newton Proposal ID #04009103

Computer Science

Supernovae, Supernova Remnants, Diffuse (Galactic) Emission And Isolated Neutron Stars, G23.5-0.0, G318.9+0.4, G25.5+0.0, Xmm-Newton Proposal 04009103

Scientific paper

Supernova Remnants of center-filled and composite types often host young, energetic pulsars emitting strong relativistic winds. Chandra and XMM-Newton observations of such SNRs have already resulted in a number of pulsar and pulsar-wind nebula (PWN) discoveries. We propose to complete the X-ray census of plerionic remnants within a 7 kpc distance, which we have begun in XMM-Newton AO-4. The SNRs were selected based on their radio morphologies and archival ROSAT or ASCA data. This short survey will substantially expand the sample of PNWe and pulsars observed in X-rays and help to establish the properties of the overall population.

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