XMM-Newton Proposal 03065101

Details XMM-Newton Proposal 03065101 XMM-Newton Proposal 03065101

Oct 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004xmm..prop..211n&link_type=abstract

XMM-Newton Proposal ID #03065101

Computer Science

Supernovae, Supernova Remnants, Diffuse (Galactic) Emission And Isolated Neutron Stars, Ctb 37A, Xmm-Newton Proposal 03065101

Scientific paper

The interaction between SNRs and molecular clouds causes immediate heating and changes the chemical composition of the surrounding gas, emitting thermal and non-thermal X-rays, OH maser lines, and gamma-rays. However, what causes the partial overlap among maser-emitting SNRs, EGRET source SNRs, SNRs with particular X-ray properties such as mixed-morphology SNRs is still unclear. CTB 37A is a radio-bright Galactic SNR, and is accompanied by OH masers and EGRET source. As the best target for the study of the SNRs in the dense conditions, we propose the wide-band and large effective area observation of CTB 37A with XMM-Newton.

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