A study of iron and dust in the supernova remnant IC 443
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文摘

We performed near-IR [Fe II] and Pa mapping of the supernova remnant IC 443 with the IRSF/SIRIUS.

We detected the [Fe II] and Pa 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.

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