2003 | OriginalPaper | Buchkapitel
The Structure of Magnetic Herbig—Haro Jets
verfasst von : Max Camenzind, Markus Thiele
Erschienen in: High Performance Computing in Science and Engineering ’02
Verlag: Springer Berlin Heidelberg
Enthalten in: Professional Book Archive
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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.