XMM-Newton Proposal 02069701

Details XMM-Newton Proposal 02069701 XMM-Newton Proposal 02069701

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003xmm..prop..356c&link_type=abstract

XMM-Newton Proposal ID #02069701

Physics

Psr J1016-5857, Xmm-Newton Proposal 02069701

Scientific paper

PSR J1016-5857 is a young and energetic pulsar located just outside the supernova remnant (SNR) G284.3-1.8. The morphology of the system argues that the pulsar has a high space velocity, and has caught up with and now overtaken its associated SNR. We have identified an Einstein source, which in the above hypothesis is likely to be a cometary nebula powered by the pulsar. We here propose to test this hypothesis with an XMM observation aimed at determining the spectrum and morphology of this X-ray emission; at the same time we will look for pulsed emission from the pulsar itself.

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