X-Ray and Radio Emission of the Galactic Supernova Remnant G7.7-3.7

Details X-Ray and Radio Emission of the Galactic Supernova Remnant G7.7-3.7 X-Ray and Radio Emission of the Galactic Supernova Remnant G7.7-3.7

Oct 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010xmm..prop...49s&link_type=abstract

XMM-Newton Proposal ID #06711701

Computer Science

Supernovae, Supernova Remnants, Diffuse (Galactic) Emission And Isolated Neutron Stars, G7.7-3.7

Scientific paper

We propose to analyse the X-ray emission of the Galactic SNR G7.7-3.7, a ~21' radio SNR with a peculiar filamentary morphology with bright knots. The X-ray emission, as detected by ROSAT and ASCA, seems to be confined to the east of the radio shell, with its intensity increasing at the location of a bright radio feature near the limb of the SNR and, interestingly, a compact X-ray source coincident with a point-like radio structure. Combining the high quality XMM and radio data will allow us to investigate the nature of the compact X-ray object and discern between different scenarios which could give rise to the peculiar morphology. The high spectral and spatial resolution X-ray data covering the complete extent of SNR will also be used to constrain its age and energetics.

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