RXJ1713.7-3946: a unique synchrotron-dominated shell-like SNR

Details RXJ1713.7-3946: a unique synchrotron-dominated shell-like SNR RXJ1713.7-3946: a unique synchrotron-dominated shell-like SNR

Oct 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007xmm..prop...35b&link_type=abstract

XMM-Newton Proposal ID #05510301

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Supernovae, Supernova Remnants, Diffuse (Galactic) Emission And Isolated Neutron Stars, Rxj1713 South, Xmm-Newton Proposal Id #05510301

Scientific paper

We propose to finish mapping the supernova remnant RX J1713.7-3946 by reobserving one 20 ks pointing which was lost to flaring activity: 1) to obtain the full and most detailed description of the morphology of the X- ray synchrotron emission to serve as a reference for other wavelengths 2) to compare how particle acceleration proceeds when the SNR is interacting with molecular clouds or with a tenuous ambient medium 3) to map the material interacting with the SNR from the variations of the X- ray absorption and compare it to the potential hadronic gamma-ray emission 4) to map accurately the spectral index variations of the X-ray synchrotron emission and look for spatial correlations with the gamma-ray spectra

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