XMM-Newton Proposal 02052603

Details XMM-Newton Proposal 02052603 XMM-Newton Proposal 02052603

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003xmm..prop..277s&link_type=abstract

XMM-Newton Proposal ID #02052603

Computer Science

Snrc J0449-6921, Snrc J0506-6541, Xmm-Newton Proposal 02052603

Scientific paper

The Large Magellanic Cloud (LMC), with its low foreground absorption and relative proximity, offers the ideal laboratory for the study of a large sample of supernova remnants (SNRs) in detail, both spatially and energetically given the known distance. It is possible to obtain a relatively complete sample of SNRs in the LMC to examine not only the global properties but the subclasses. Toward this goal, we are identifying new SNRs using combined optical, radio, and X-ray data. Here we request XMM-Newton observations of six intriguing SNR candidates which probe different interstellar environments. These objects lend themselves to a study of the relationships between environment and SNR properties in addition to the detailed individual analysis of each object.

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