XMM-Newton Proposal 03031002

Details XMM-Newton Proposal 03031002 XMM-Newton Proposal 03031002

Oct 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004xmm..prop..112h&link_type=abstract

XMM-Newton Proposal ID #03031002

Computer Science

Supernovae, Supernova Remnants, Diffuse (Galactic) Emission And Isolated Neutron Stars, G337.8-0.1, G304.6+0.1, Xmm-Newton Proposal 03031002

Scientific paper

We propose to continue our study of a small sample of Galactic supernova remnants that we have recently discovered to be X-ray emitters. The sample consists of ejecta-dominated SNRs as well as ones with normal composition. The proposed XMM observations will be an order of magnitude deeper than existing X-ray data. The specific goals of the XMM study are to (1) measure accurate values for the elemental abundances, (2) determine the evolutionary state of the remnants from their X-ray emission properties (e.g., temperature, ionization timescale, flux), and (3) search for hard X-ray sources that might be pulsars or pulsar wind nebulae.

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