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The Jet of HH34: New Results

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Mass Outflows from Stars and Galactic Nuclei

Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 142))

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Abstract

Narrow band filter imaging of the HH34 jet system reveals an inhomogeneous excitation structure in HH34, in particular a compact [OIII] -emission region near the apex of the bow shock. About 2′ N of the jet source a counter bow shock was discovered of very similar appearance to HH34. Long-slit spectroscopy with high resolution shows a two velocity component flow in the jet and an inhomogeneous velocity structure in HH34. These phenomena are briefly discussed in terms of interactions of the flow with the surrounding medium and/or thermal instabilities in the cooling regions of a bow shock.

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References

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Author information

Authors and Affiliations

  1. Max-Planck-Institut für Astronomie, Königstuhl, 6900, Heidelberg, Germany

    Th. Bührke

Authors
  1. Th. Bührke
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Editor information

Editors and Affiliations

  1. Osservatorio Astronomico di Torino, Pino Torinese, Italy

    Luciana Bianchi

  2. ESA/VILSPA, IUE Groundstation, Madrid, Spain

    Roberto Gilmozzi

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© 1988 Kluwer Academic Publishers

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Bührke, T. (1988). The Jet of HH34: New Results. In: Bianchi, L., Gilmozzi, R. (eds) Mass Outflows from Stars and Galactic Nuclei. Astrophysics and Space Science Library, vol 142. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-2941-8_42

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  • DOI: https://doi.org/10.1007/978-94-009-2941-8_42

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-7824-5

  • Online ISBN: 978-94-009-2941-8

  • eBook Packages: Springer Book Archive

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