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Optical emission-line jets in star formation regions

  • Part I: The Physics of Interstellar Molecular Clouds: Individual Regions
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Book cover The Physics and Chemistry of Interstellar Molecular Clouds: mm and Sub-mm Observations in Astrophysics

Part of the book series: Lecture Notes in Physics ((LNP,volume 331))

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Abstract

The morphological and kinematical properties of optical emission-line jets and related collimated “optical” flows from young stellar objects are reviewed. Some recently obtained high-quality CCD images are displayed to illustrate the morphological properties of these flows and their associated bow-shock like structures. The available data on the driving sources of these flows are also reviewed.

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Authors and Affiliations

  1. Max-Planck-Institut für Astronomie, Königstuhl 17, 6900, Heidelberg, Fed. Rep. of Germany

    Reinhard Mundt

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  1. Reinhard Mundt
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© 1989 Springer-Verlag Berlin Heidelberg

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Mundt, R. (1989). Optical emission-line jets in star formation regions. In: The Physics and Chemistry of Interstellar Molecular Clouds: mm and Sub-mm Observations in Astrophysics. Lecture Notes in Physics, vol 331. Springer, Berlin, Heidelberg. https://doi.org/10.1007/BFb0119470

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  • DOI: https://doi.org/10.1007/BFb0119470

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  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-540-51297-4

  • Online ISBN: 978-3-540-46187-6

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