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Topological Solutions for Collimated MHD Flows

  • K. Tsinganos (a1) and E. Trussoni (a2)

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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.

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References

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

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