XMM-Newton Proposal 02051401

Details XMM-Newton Proposal 02051401 XMM-Newton Proposal 02051401

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003xmm..prop..270l&link_type=abstract

XMM-Newton Proposal ID #02051401

Computer Science

W51C Center, Xmm-Newton Proposal 02051401

Scientific paper

W51B+C is one of the few regions in the Galaxy where we can study the formation of massive stars and the consequence of their violent explosions simultaneously. It is composed of an active star forming region, W51B, and an old SNR, W51C. There is strong evidence suggesting that the SNR is interacting with the star-forming molecular clouds. We have done Chandra observations and identified several interesting features including a promising candidate for pulsar/PWN, bright (evaporating?) clumps in soft X-rays, and hard X-ray emission from star-forming regions. The purpose of this proposal is to obtain sensitive XMM/Newton spectra of these sources for spatially-resolved spectral analysis.

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