Self-Collimated Stationary Disk Winds

Ferreira, Jonathan; Casse, Fabien

doi:10.1007/978-94-017-0491-5_35

Self-Collimated Stationary Disk Winds

Jonathan Ferreira⁷ &
Fabien Casse⁸

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Abstract

In this contribution, we first review the theory of self-collimated jets launched from magnetized accretion disks (disk-winds originating from the first AUs). We show why it is crucial to solve in a self-consistent way the interplay between the resistive accretion disk and the ideal MHD jets. Indeed, this is the only way to get exact values for the disk ejection efficiency ξ (the jet mass load issue). Then, we show self-similar calculations of such accretion-ejection structures: first cold jets, then warm jets obtained in the presence of a hot disk chromosphere. Finally, we present for the first time an accretion-ejection flow crossing all three critical points.

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Authors and Affiliations

Laboratoire d’Astrophysique de Grenoble, Grenoble Cedex, France
Jonathan Ferreira
FOM-Institute for Plasma Physics “Rijnhuizen”, Nieuwegein, The Netherlands
Fabien Casse

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Jonathan Ferreira
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Fabien Casse
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Editors and Affiliations

Instituto de Astronomía y Geodesia (CSIC-UCM), Universidad Complutense de Madrid, Spain
A. I. Gómez de Castro
University of Massachussetts, Amherst, MA, USA
M. Heyer
Centro de Radioastronomía y Astrofísica, UNAM, 58089, Morelia, Michoacán, Mexico
E. Vázquez-Semadeni
Instituto de Astrofísica de Canarias, La Laguna, Tenerife, Spain
R. Rebolo
Service d’Astrophysique, CEA-Saclay, Gif-sur-Yvette, France
M. Tagger
McMaster University, Hamilton, ON, Canada
R. E. Pudritz

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Ferreira, J., Casse, F. (2004). Self-Collimated Stationary Disk Winds. In: de Castro, A.I.G., Heyer, M., Vázquez-Semadeni, E., Rebolo, R., Tagger, M., Pudritz, R.E. (eds) Magnetic Fields and Star Formation. Springer, Dordrecht. https://doi.org/10.1007/978-94-017-0491-5_35

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DOI: https://doi.org/10.1007/978-94-017-0491-5_35
Publisher Name: Springer, Dordrecht
Print ISBN: 978-90-481-6602-2
Online ISBN: 978-94-017-0491-5
eBook Packages: Springer Book Archive

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