Searching for compact central source in the radio supernova remanent MSH 10 53S

Details Searching for compact central source in the radio supernova remanent MSH 10 53S Searching for compact central source in the radio supernova remanent MSH 10 53S

Oct 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008xmm..prop..124d&link_type=abstract

XMM-Newton Proposal ID #06047001

Computer Science

Supernovae, Supernova Remnants, Diffuse (Galactic) Emission And Isolated Neutron Stars, Msh 10-53/Snr G

Scientific paper

A significant excess of very high energy (VHE) gamma-ray emission is observed by H.E.S.S. inside the shell of SNR G284.3--1.8. This source is found to be point-like or only slightly extended and at a distance of 0.33d from PSR J1016-5857. A 1.8 ks Einstein observation reveal a significant excess compatible with the VHE source. This association suggests that this could be the actual PWN of MSH 10-53. The estimated flux suggests that this object should be easily detectable by XMM-Newton.

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