On the observed infrared fluxes from extragalactic H II regions

The authors calculate, for extragalactic H II regions, the expected relationship between the radio flux at 11 cm and the infrared flux at 11 and 20 μm based on the grain models and the parameters which fit the observations of galactic H II regions. It is shown that the measured infrared fluxes of extragalactic H II regions are consistent with the expected infrared fluxes for these objects. (Auth.)