Paper:	Hard X-ray Emission From the IC 443 SNR
Volume:	271, Neutron Stars in Supernova Remnants
Page:	403
Authors:	Bocchino, F.; Bykov, A.
Abstract:	We present XMM observations of hard X-ray emission from the field of IC 443 a supernova remnant interacting with a molecular cloud. The hard emission from the field is dominated by 12 isolated sources having 2-10 keV flux higher than 5 x 10-14 erg/cm2/s. Some of the sources are expected to be related to the SNR, given their positional coincidence with infrared emission associated to the interaction between the shock and a molecular cloud. We present a spectral study of the brightest sources. We also present upper limits on the nonthermal diffuse X-ray emission of radio emitting electrons accelerated by SNR shock wave in the northeastern ridge.

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