paper

Spitzer Observations of M83 and the Hot Star, H II Region Connection

arXiv:astro-ph/0703217 · doi:10.1111/j.1365-2966.2007.11714.x

Abstract

We have undertaken a program to observe emission lines of SIV 10.5, NeII 12.8, NeIII 15.6, & SIII 18.7 um in a number of extragalactic HII regions with the Spitzer Space Telescope. We report our results for the nearly face-on spiral galaxy M83. The nebulae selected cover a wide range of galactocentric radii (R_G). The observations were made with the Infrared Spectrograph in the short wavelength, high dispersion configuration. The above set of 4 lines is observed cospatially, thus permitting a reliable comparison of the fluxes. From the measured fluxes, we determine the ionic abundance ratios including Ne++/Ne+, S3+/S++, and S++/Ne+ and find that there is a correlation of increasingly higher ionization with larger R_G. By sampling the dominant ionization states of Ne and S for HII regions, Ne/S ~ (Ne+ + Ne++)/(S++ + S3+). Our findings of ratios that exceed the benchmark Orion value are more likely due to other effects than a true gradient in Ne/S. Both Ne and S are primary elements produced in alpha- chain reactions. It is expected that Ne/S remains relatively constant throughout a galaxy. This type of observation and method of analysis has the potential for accurate measurements of Ne/S, particularly for HII regions with lower metallicity & higher ionization than those here, such as those in M33. Our observations may also be used to test the predicted ionizing spectral energy distribution of various stellar atmosphere models. We compare the fractional ionization ratios <Ne++>/<S++> & <Ne++>/<S3+> vs. <S3+>/<S++> with predictions made from our photoionization models using several state-of-the-art stellar atmosphere model grids. A second paper using Spitzer observations of HII regions in the galaxy M33 will follow.

arXiv commentAccepted MNRAS: 31 pages, 7 figures, 3 tables

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