Chandra and XMM-Newton Observations of Young Supernova Remnants

Details Chandra and XMM-Newton Observations of Young Supernova Remnants Chandra and XMM-Newton Observations of Young Supernova Remnants

Jun 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aas...208.6103s&link_type=abstract

American Astronomical Society Meeting 208, #61.03; Bulletin of the American Astronomical Society, Vol. 38, p.141

Astronomy and Astrophysics

Astronomy

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Scientific paper

Supernova Remnants (SNRs) provide excellent targets to probe the energetics of the supernova explosions, the production of heavy elements, the formation of compact objects, the interaction between their fast-moving shocks and the surrounding medium, and the physical conditions of the ISM in which they are expanding. I will highlight X-ray studies with Chandra and XMM-Newton of a small sample of young (a few thousand year-old) SNRs targeted to address the above-mentioned science. These SNRs include targets discovered at radio wavelengths with the Canadian Galactic Plane Survey.

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