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The Structure of Magnetic Herbig—Haro Jets

In: High Performance Computing in Science and Engineering ’02

Author

Listed:
  • Max Camenzind

    (Landessteriiwarte Königstuhl)

  • Markus Thiele

    (Landessteriiwarte Königstuhl)

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.

Suggested Citation

  • Max Camenzind & Markus Thiele, 2003. "The Structure of Magnetic Herbig—Haro Jets," Springer Books, in: Egon Krause & Willi Jäger (ed.), High Performance Computing in Science and Engineering ’02, pages 62-69, Springer.
  • Handle: RePEc:spr:sprchp:978-3-642-59354-3_5
    DOI: 10.1007/978-3-642-59354-3_5
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