XMM-Newton Proposal 03069101

Details XMM-Newton Proposal 03069101 XMM-Newton Proposal 03069101

Oct 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004xmm..prop..222c&link_type=abstract

XMM-Newton Proposal ID #03069101

Mathematics

Logic

Supernovae, Supernova Remnants, Diffuse (Galactic) Emission And Isolated Neutron Stars, Psr J1357-6429, Xmm-Newton Proposal 03069101

Scientific paper

PSR J1357-6429 is a very young (7 kyr) and nearby (~2.5 kpc) energetic radio pulsar apparently associated with the supernova remnant candidate G309.8-2.6. The only existing X-ray observations of this system were obtained in the ROSAT All-Sky Survey that apparently show a bright extended source positionally coincident with the pulsar and with a candidate supernova remnant detected at radio wavelengths. We here propose a short XMM observation in order to establish the basic properties of this system. If, as expected, this is a bright X-ray source, the requested 10 ksec observation should begin to reveal spectroscopic and morphological details of the pulsar wind nebula/pulsar and form the basis for future more detailed studies.

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