Evolution of H ii regions in hierarchically structured molecular clouds

• Published in: Monthly notices of the Royal Astronomical Society Vol. 372; no. 1; pp. 457 - 466
• Main Authors: Shabala, S. S., Ellingsen, S. P., Kurtz, S. E., Forbes, L. K.
• Format: Journal Article
• Language: English
• Published: Oxford, UK Blackwell Publishing Ltd 11.10.2006; Blackwell Science; Oxford University Press
• Subjects: Astronomy; Clouds; Earth, ocean, space; Emissions; Exact sciences and technology; Gases; H ii regions; ISM: structure; radio lines: ISM; Stars & galaxies; stars: formation; H; stars: formation; regions; radio lines: ISM; ISM: structure; Ionized gases; Molecular clouds; Recombination line; HII regions; H II regions; Star formation; Masers; Physical parameter; Density gradient; Emission measure; Emission line; Age; Hydrostatic model; Methanol
• ISSN: 0035-8711; 1365-2966
• DOI: 10.1111/j.1365-2966.2006.10883.x

We present observations of the H91α recombination line emission towards a sample of nine H ii regions associated with 6.7-GHz methanol masers, and report arcsecond-scale emission around compact cores. We derive physical parameters for our sources, and find that although simple hydrostatic models of region evolution reproduce the observed region sizes, they significantly underestimate emission measures. We argue that these findings are consistent with young source ages in our sample, and can be explained by existence of density gradients in the ionized gas.