Point-Like and Extended X-Ray Sources in the Supernova Remnant IC443

Details Point-Like and Extended X-Ray Sources in the Supernova Remnant IC443 Point-Like and Extended X-Ray Sources in the Supernova Remnant IC443

Feb 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005tmgm.meet.1268b&link_type=abstract

The Tenth Marcel Grossmann Meeting. Proceedings of the MG10 Meeting held at Brazilian Center for Research in Physics (CBPF), Rio

Physics

Scientific paper

We present the results we have obtained on the non-thermal hard X-ray emission from IC443, a supernova remnant interacting with molecular cloud (MC), from the initial discovery with BeppoSAX/PDS to the most recent results with XMM/Newton. This remnant has been detected up to EGRET bandwidth, and we have resolved part of the hard emission as 1) a plerion nebula with a compact central object, 2) a set of isolated point sources in the MC interaction regions, and 3) a diffuse extended component. We introduce the models we have invoked to explain all these components and the problems still open.

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