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Estimating the Porosity of the Interstellar Medium from Three Dimensional Photoionization Modeling of H II Regions

By Kenneth Wood, LM Haffner, RJ Reynolds, JS Mathis and G Madsen
Topics: HII regions, ISM : structure, radiative transfer, stars : individual (xi Ophiuchi), DIFFUSE IONIZED-GAS, EDGE-ON GALAXIES, MILKY-WAY, PHYSICAL CONDITIONS, MOLECULAR CLOUDS, SPIRAL GALAXIES, ZETA-OPHIUCHI, HII-REGIONS, IONIZATION, EMISSION
Year: 2005
DOI identifier: 10.1086/432831
OAI identifier: oai:risweb.st-andrews.ac.uk:publications/5bf2147b-43e4-4cf6-ad34-c6d783ca7493
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