We performed near-IR [Fe II] and Pa尾 mapping of the supernova remnant IC 443 with the IRSF/SIRIUS.
We detected the [Fe II] and Pa尾 emissions from a very wide area of IC 443.
From inner parts where [Fe II] is detected but dust is not, we detected 6.7 keV Fe emission with Suzaku.
From the maps of the [Fe II], He-like Fe, and dust, we discuss the properties of Fe-bearing dust.