An XMM-Newton Study of the Supernova Remnant G296.1-0.5

Details An XMM-Newton Study of the Supernova Remnant G296.1-0.5 An XMM-Newton Study of the Supernova Remnant G296.1-0.5

Oct 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006xmm..prop..120s&link_type=abstract

XMM-Newton Proposal ID #05032203

Computer Science

Supernovae, Supernova Remnants, Diffuse (Galactic) Emission And Isolated Neutron Stars, G296.1-0.5 P1, G296.1-0.5 P2, G296.1-0.5 P3, Xmm-Newton Proposal 05032203

Scientific paper

G292.1-0.5 is a bright, relatively nearby supernova remnant whose spectrum and morphology indicate complex shock structures and a possible interaction dense ambient material. A partial-shell morphology is accompanied by a multicomponent spectrum whose properties may be associated with reflected shocks from an interaction with dense material, or with nonthermal particles accelerated to cosmic-ray energies. The low absorption and high luminosity make this an important remnant for the study of such processes. In addition, important constraints can be placed on any associated neutron star. We propose XMM-Newton observations to provide full coverage of this SNR in order to study in detail the spectrum and morphology, and to search for an associated neutron star.

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