XMM-Newton Proposal 02036502

Details XMM-Newton Proposal 02036502 XMM-Newton Proposal 02036502

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003xmm..prop..190s&link_type=abstract

XMM-Newton Proposal ID #02036502

Physics

Psr J1524-5625, Psr J0940-5428, Xmm-Newton Proposal 02036502

Scientific paper

Young (characteristic age 10-100 kyr) pulsars represent a transition group from very young pulsars, characterized by strong nonthermal radiation and bright synchrotron pulsar wind nebulae, to middle aged pulsars, characterized by the thermal radiation. The investigation of young pulsars allows us to understand this transition and constrain the parameters responsible for pulsar evolution. Pulsars recently discovered in the Parkes Multibeam survey provide an opportunity to increase the number of X-ray observed young pulsars. We propose to observe four such young pulsars utilizing the superior sensitivity of the XMM-Newton.

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