Iron abundance in Galactic H II regions

Astronomy and Astrophysics – Astronomy

Scientific paper

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Dust, Extinction, H Ii Regions, Ism: Abundances

Scientific paper

Some recent results point to a possible discrepancy between the Fe abundance in M42 as derived from the emission of the different Fe ions, but it is argued that the uncertainties are currently too high to decide whether the discrepancy is real. The results of a recent analysis of the Fe abundance in 7 Galactic H II regions are discussed as well as the implications they could have for dust in H II regions.

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