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Topological Solutions for Collimated MHD Flows

Published online by Cambridge University Press:  19 July 2016

K. Tsinganos  and
E. Trussoni
K. Tsinganos
Affiliation:
(1)Department of Physics, University of Crete, Heraklion, Greece
E. Trussoni
Affiliation:
(2)Istituto di Cosmo-geofisica del C.N.R., Torino, Italy

Extract

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Different astrophysicai contexts (e.g. extragalactic jets, star forming regions) are related with collimated ouflows. An analysis of this phenomenology in principle would require a fully numerical treatment, however analytical investigations are also possible by assuming a suitable behaviour of streamlines. In this framework we investigate solutions of the hydrodynamic and MHD equations describing helicoidal collimated outflows from a central gravitating object.

Type
6. Magnetic Fields in Molecular Clouds, Dark Globules and in the Pre-Stellar and Circumstellar Environment
Information
Symposium - International Astronomical Union , Volume 140: Galactic and Intergalactic Magnetic Fields , 1990 , pp. 333 - 336
Copyright
Copyright © Kluwer 1990 

References

Tsinganos, K. and Trussoni, E.: 1989, Astron. Astrophys. , submitted Weber, E.J. and Davis, L.: 1967, Astrophys. J. 148, 217.Google Scholar