Spatial Distribution of Dust Grains within H Ii Regions

We discuss the dust distribution within photoionized regions. Assuming a geometry with a central dust cavity, which is strongly suggested by the literature, we can estimate the cavity’s radius from the ratio of the infrared and radio fluxes by using a simple transfer model of Lyman continuum photons. We apply the method to a sample of the Galactic H ii regions. The estimated typical radius of the dust cavity of the Galactic compact H ii regions is about 30% of the Strömgren radius. Taking account of uncertainties both of the observational data and the model, we can reject a dust distribution lacking a central cavity. Therefore, the dust cavity model is supported independently of the previous works. We discuss the formation mechanism of such a dust cavity and its detectability by present and future infrared facilities. Subject headings: dust, extinction — H II regions — infrared: ISM — radiative transfer — submillimeter