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• W1663399719 abstract "We carried out a series of 1D hydrodynamical computations with the ZEUS fluid solver in order to reproduce the salient features in our high-resolution Hα emission line profiles of a sample of HII regions (see Rozas et al. 2006a,b). Four models were computed. In the first and second cases, an ionization-bounded HII region was modeled with and without a shell produced by stellar winds. In the third and fourth cases, a density-bounded HII region was considered, both with and without a shell driven by stellar winds. The resulting line profiles have been modeled using the SHAPE rendering program. We find that our observed high-quality profiles are well-reproduced in the density-bounded model that includes an expanding shell formed as a result of the stellar winds from the ionizing stars. Finally, we consider the effects that the finite slit widths used for the observations have on the physical conditions deduced from the line profile of the ionized bubble." @default.
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• W1663399719 date "2006-11-02" @default.
• W1663399719 modified "2023-10-17" @default.
• W1663399719 title "H<i>α</i>line profiles for a sample of supergiant HII regions" @default.
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• W1663399719 doi "https://doi.org/10.1051/0004-6361:20065262" @default.
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