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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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
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