Hostname: page-component-586b7cd67f-t7czq Total loading time: 0 Render date: 2024-11-26T22:13:10.125Z Has data issue: false hasContentIssue false
  • English
  • Français

Self-Similar MHD Collimated Outflows

Published online by Cambridge University Press:  12 April 2016

E. Trussoni ,
C. Sauty  and
K. Tsinganos
E. Trussoni
Affiliation:
Osservatorio Astronomico di Torino, Pino Torinese, Italy
C. Sauty
Affiliation:
Observatoire de Paris, DAEC, Meudon, France
K. Tsinganos
Affiliation:
University of Crete, Dept. of Physics, Heraklion, Greece

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We present a class of steady axisymmetric MHD solutions, self-similar in the meridional direction, that are suitable to model collimated winds accelerated in the potential well of a spherical object.

Type
Part 15. Poster Papers
Information
International Astronomical Union Colloquium , Volume 163: Accretion Phenomena and Related Outflows , 1997 , pp. 816 - 817
Copyright
Copyright © Astronomical Society of the Pacific 1997

References

Blandford, R.D & Payne, D.G. 1982, MNRAS, 199, 883 CrossRefGoogle Scholar
Trussoni, E., Sauty, C. & Tsinganos, K. 1996, in Solar and Astrophysical MHD Flows, Tsinganos, K. (ed.), Kluwer Academic Publishers, 383 Google Scholar