Computer Science
Scientific paper
Mar 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003xmm..prop..204h&link_type=abstract
XMM-Newton Proposal ID #02038502
Computer Science
G30.8-0.0, G24.3+0.0, Xmm-Newton Proposal 02038502
Scientific paper
The recent detection of several diffuse, hard-X-ray sources in the ASCA Galactic plane survey provides new candidates in the search for the dozens of young, Crab-like remnants missing from the current Milky Way supernova remnant catalog. By comparing this survey with our new VLA survey of the Galactic plane, we have discovered two strong candidates for young pulsar wind nebulae. We propose to image both objects with XMM to confirm their nature and measure the source properties.
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