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- W1574674694 abstract "We critically examine stellar atmosphere models by exploiting the strong dependence of H II region optical spectra on the SED of the ionizing source. To accomplish this, we compare spatially resolved, longslit observations of LMC single-star H II regions to photoionization simulations based on observed nebular and stellar properties. We select stellar atmosphere models from the CoStar (Schaerer & de Koter, 1997), TLUSTY (Lanz & Hubeny, 2003), WM-basic (Pauldrach et al. 2001) and Smith et. al. (2002) grids to define the ionizing source in our simulations. Gas density fluctuations are necessary to simultaneously fit the emission from high and low excitation ions. We evaluate the atmospheres relative to each other and overall, find atmosphere models using the WM-basic code have the best agreement with our observations." @default.
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- W1574674694 date "2011-01-17" @default.
- W1574674694 modified "2023-09-24" @default.
- W1574674694 title "Single-Star HII Regions as a Probe of Massive Star SEDs" @default.
- W1574674694 hasPublicationYear "2011" @default.
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