XMM-Newton Proposal 03021901

Details XMM-Newton Proposal 03021901 XMM-Newton Proposal 03021901

Oct 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004xmm..prop...77m&link_type=abstract

XMM-Newton Proposal ID #03021901

Physics

Supernovae, Supernova Remnants, Diffuse (Galactic) Emission And Isolated Neutron Stars, Vela File, Xmm-Newton Proposal 03021901

Scientific paper

This proposal is part of a multi-wavelength survey of the Vela SNR which intends to test the different models of shock-cloud interaction in the SNRs. We propose to observe a bright region in the northern rim of the Vela shell, already included in a recently approved ESO proposal. The selected region presents all the characteristic features of the shock-cloud interaction and the study of its X-ray emission, together with the analysis of available EPIC observations of two adjacent regions, will allow us to obtain a complete high spatial resolution scenario of the shocked plasma in this part of the Vela SNR. The X-ray data will be compared also with photometric and spectroscopic optical data of the same region to obtain important constraints for the physics of the shocked plasma.

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