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Evolution of H ii regions in hierarchically structured molecular clouds
Authors:S. S. Shabala  S. P. Ellingsen  S. E. Kurtz   L. K. Forbes
Affiliation:School of Mathematics and Physics, University of Tasmania, Private Bag 21, Hobart, Tasmania 7001, Australia;Astrophysics Group, Cavendish Laboratory, Madingley Road, Cambridge CB3 0HE;Centro de Radioastronomía y Astrofísica, UNAM, Apdo Postal 3-72, CP 58089, Morelia, Michoacán, México
Abstract:
Keywords:stars: formation    H ii regions    ISM: structure    radio lines: ISM
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