Searching for PWNe in three center-filled Supernova Remnants

Details Searching for PWNe in three center-filled Supernova Remnants Searching for PWNe in three center-filled Supernova Remnants

Oct 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007xmm..prop...98k&link_type=abstract

XMM-Newton Proposal ID #05531103

Computer Science

Supernovae, Supernova Remnants, Diffuse (Galactic) Emission And Isolated Neutron Stars, G83.0-0.3, G341.2+0.9, G94.0+1.0, Xmm-Newton Proposal Id #05531103

Scientific paper

Supernova Remnants of center-filled and composite types often host young, energetic pulsars emitting strong relativistic winds. XMM-Newton and Chandra observations of such SNRs have already resulted in a number of pulsar and pulsar-wind nebula (PWN) discoveries. We propose to observe three plerionic remnants located within a 7 kpc distance. The SNRs were selected based on their radio morphologies and archival ROSAT data. We expect to expand the limited sample of X-ray bright PWNe suitable for detailed X-ray studies.

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