All’s Knot Quiet on the Recombination Front

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Shocks in Astrophysics

Abstract

Molecular clouds are clumpy on length scales down to the limits of observational resolution. At least some ultracompact Hii regions (UCHiiR) may result from the interaction of a young early type star and this type of cloud. The clumps can act as reservoirs of ionized gas distributed within the Hii region. These models reproduce the relatively long lifetimes implied by the population statistics of UCHiiR. We present line profile and emission measure plots based on the simplest case where the flow remains supersonic through to a recombination front. The morphology agrees with the shell-like UCHiiR as classified by Churchwell. The predicted line profiles are broad and double peaked with a separation of about 50 km s−1 for the example given.

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© 1995 Kluwer Academic Publishers

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Redman, M.P., Williams, R.J.R., Dyson, J.E. (1995). All’s Knot Quiet on the Recombination Front. In: Millar, T.J., Raga, A.C. (eds) Shocks in Astrophysics. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-1624-1_27

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  • DOI: https://doi.org/10.1007/978-94-009-1624-1_27

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-7225-0

  • Online ISBN: 978-94-009-1624-1

  • eBook Packages: Springer Book Archive

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