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Interaction of the HII Region S236 with the Surrounding Medium

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Regions of Recent Star Formation

Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 93))

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Abstract

The HII region S236 has been observed in the continuum at 50 cm wavelength and in the recombination line H166α at 10 selected positions. A mean electron temperature Te = 7600 K is derived for the nebula and the measured velocity pattern is explained qualitatively in terms of a gas flow from the molecular cloud.

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References

  • Blitz, L.: 1980, private communication

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  • Churchwell, E.: 1980, in “Radio Recombination Lines”, Ed. P.A. Shaver, D. Reidel, Dordrecht p. 225

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  • Donati Falchi, A., Felli, M., Tofani, G.: 1980, Astron. Astrophys. 89, p. 363

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  • Georgelin, Y.M.: 1975, Ph. D. Thesis, Université de Provence, Marseille, France

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Author information

Authors and Affiliations

  1. Arcetri Astrophysical Observatory, Florence, Italy

    A. Falchi & G. Tofani

  2. Radiosterrenwacht, Dwingeloo, The Netherlands

    R. H. Harten

Authors
  1. A. Falchi
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  2. G. Tofani
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  3. R. H. Harten
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Editor information

Editors and Affiliations

  1. Dominion Radio Astrophysical Observatory, Herzberg Institute of Astrophysics, National Research Council of Canada, Penticton, B.C., Canada

    R. S. Roger  & Peter E. Dewdney  & 

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© 1982 D. Reidel Publishing Company

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Falchi, A., Tofani, G., Harten, R.H. (1982). Interaction of the HII Region S236 with the Surrounding Medium. In: Roger, R.S., Dewdney, P.E. (eds) Regions of Recent Star Formation. Astrophysics and Space Science Library, vol 93. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-7778-5_5

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  • DOI: https://doi.org/10.1007/978-94-009-7778-5_5

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-009-7780-8

  • Online ISBN: 978-94-009-7778-5

  • eBook Packages: Springer Book Archive

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