Infrared Dust Bubbles: Probing the Detailed Structure and Young Massive Stellar Populations of Galactic H II Regions

@article{Watson2008InfraredDB,
  title={Infrared Dust Bubbles: Probing the Detailed Structure and Young Massive Stellar Populations of Galactic H II Regions},
  author={Christer Watson and Matthew S. Povich and Edward Bruce Churchwell and Brian L. Babler and Georgi Chunev and M. G. Hoare and R{\'e}my Indebetouw and M. R. Meade and Thomas P. Robitaille and Barbara. A. Whitney},
  journal={The Astrophysical Journal},
  year={2008},
  volume={681},
  pages={1341 - 1355}
}
We present an analysis of wind-blown, parsec-sized, mid-infrared bubbles and associated star formation using the GLIMPSE IRAC, MIPSGAL MIPS, and MAGPIS VLA surveys. Three bubbles from the Churchwell et al. catalog were selected. The relative distribution of the ionized gas (based on 20 cm emission), PAH emission (based on 8 μm, 5.8 μm, and lack of 4.5 μm emission), and hot dust (24 μm emission) is compared. At the center of each bubble there is a region containing ionized gas and hot dust… 
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