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Mass Flux and Toroidal Magnetic Field in Magnetically Driven Jets from Accretion Disks: Steady Solutions and Application to Jet/Wind in YSO

Published online by Cambridge University Press:  12 April 2016

T. Kudoh  and
K. Shibata
T. Kudoh
Affiliation:
National Astronomical Observatory of Japan, 2-21-1, Osawa, Mitaka, Tokyo, 181, Japan
K. Shibata
Affiliation:
National Astronomical Observatory of Japan, 2-21-1, Osawa, Mitaka, Tokyo, 181, Japan

Abstract

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We solved one-dimensional steady and axisymmetric magnetohydrodynamical (MHD) equations to study basic properties of astrophysical jets from accretion disks. We found that the mass flux of the jets depends on the poloidal magnetic field strength of the disk. The mass loss rates observed in T Tauri winds will constrain the physical quantities in the accretion disks.

Type
Part 15. Poster Papers
Information
International Astronomical Union Colloquium , Volume 163: Accretion Phenomena and Related Outflows , 1997 , pp. 751 - 752
Copyright
Copyright © Astronomical Society of the Pacific 1997

References

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