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Paper: Modeling the Ultracompact HII Regions and Comparison with ISO Mid-Infrared Spectroscopy
Volume: 267, Hot Star Workshop III: the Earliest Stages of Massive Star Birth
Page: 441
Authors: Watarai, H.
Abstract: Photo-ionization and dust shell models of ultracompact HII region are presented. The model predictions are directly compared with observed properties (e.g., line intensities, continuum emission from dust) obtained by ISO mid-infrared spectroscopy, and the characteristics of the embedded ionizing star(s) and the dust distribution are reported for the observed HII regions.
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