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Structure and Dynamics of the Interstellar medium pp 80–95Cite as

Turbulent and ordered motions in HII regions

  • Molecular Clouds, Star Formation And HII Regions
  • Conference paper
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Part of the book series: Lecture Notes in Physics ((LNP,volume 350))

Abstract

The HII regions morphology have suggested, from the beginning of this century, the evidence of internal motions, very few gas radial velocities (RV) on the brightest “nebulae” had been obtained, because of obvious technical difficulties. The modern Fabry-Perot interferometers and the new Integral Field Spectrograph provide abundant RV fields at various scales in the interstellar gas. New ways in imagery, owing to these new instruments, lead to a better analyse of both, the velocities field and their precise morphology free of stellar, dusty, and non thermal continua. The richness and the quality of RV data, a better understanding of the expansion phenomena authorize again a rebirth of the turbulence observations of the ionized interstellar gas.

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Authors and Affiliations

  1. Laboratoire d’Astronomie Spatiale, CNRS - Trav. du Siphon, 13012, Marseille

    G. Courtès

  2. Observatoire de Marseille, 2, Place Le Verrier, 13004, Marseille, France

    G. Courtès

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  1. G. Courtès
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Editor information

Guillermo Tenorio-Tagle Mariano Moles Jorge Melnick

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© 1989 Springer-Verlag

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Courtès, G. (1989). Turbulent and ordered motions in HII regions. In: Tenorio-Tagle, G., Moles, M., Melnick, J. (eds) Structure and Dynamics of the Interstellar medium. Lecture Notes in Physics, vol 350. Springer, Berlin, Heidelberg. https://doi.org/10.1007/BFb0114843

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  • DOI: https://doi.org/10.1007/BFb0114843

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  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-540-51956-0

  • Online ISBN: 978-3-540-46865-3

  • eBook Packages: Springer Book Archive

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