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Abstract

We present simulations of magnetized Herbig-Haro flows of low-mass stars. These slightly overdense jets propagate with about 300 km/s through the inner part of a molecular cloud. The magnetic field is injected from the central star and evolves a complicated time-dependent structure driven by pinch and kink modes. The high spatial resolution achieved on the NEC SX-5 provides for the first time insight into the phenomenon of current filamentation and the complex internal structure of pinch and kink modes.

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References

  1. Bacciotti, F., Mündt, R., Ray, T.P., Eisloeffel, J., Solf, J., Camenzind, M.: Hubble Space Telescope STIS Spectroscopy of the Optical Outflow from DG Tauri: Structure and Kinematics on Subarcsecond Scales. ApJ Lett 537 (2000) 49 -

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  2. Camenzind, M.: Energetics, Collimation and Propagation of Galactic Protostellar Outflows, in IAU Symp.182 Herbig-Haro Flows and the Birth of Low Mass Stars, ed. B. Reipurth and C. Bertout, Kluwer (Dordrecht), p. 241–258

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  3. Camenzind, M.: Imprints of Magnetic Fields, inFormation and Propagation of Young Stellar Jets, eds. E. Guenther, ASP Conf. Series188 129 -

    Google Scholar 

  4. Thiele, M.: Numerische Simulationen protostellar Jets. Dissertation, University of Heidelberg 2000

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  5. Thiele, M., Camenzind, M.: Propagation of Herbig-Haro jets through inhomogeneous molecular clouds, inHigh Performance Computing in Science and Engineering 2001, Springer-Verlag (Heidelberg), 80–91

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  6. Thiele, M., Camenzind, M.: Knot production in magnetized Herbig-Haro jets. A&A 381 (2002) L53–56

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  7. Ziegler, U.: Dissertation, University Würzburg 1995

    Google Scholar 

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© 2003 Springer-Verlag

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Camenzind, M., Thiele, M. (2003). The Structure of Magnetic Herbig—Haro Jets. In: Krause, E., Jäger, W. (eds) High Performance Computing in Science and Engineering ’02. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-59354-3_5

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  • DOI: https://doi.org/10.1007/978-3-642-59354-3_5

  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-642-63947-0

  • Online ISBN: 978-3-642-59354-3

  • eBook Packages: Springer Book Archive

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