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Electromagnetic Jets Driven by Accretion Disks

Published online by Cambridge University Press:  04 August 2017

Osamu Kaburaki  and
Motoyoshi Itoh
Osamu Kaburaki
Affiliation:
Astronomical Institute, Faculty of Science, Tohoku University, Sendai, Japan
Motoyoshi Itoh
Affiliation:
Astronomical Institute, Faculty of Science, Tohoku University, Sendai, Japan

Abstract

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As a model of ionized jets from young stars, an analytic solution has been derived from the resistive MHD equations. The essence of our model and an outline of the calculation are presented.

Type
I. Star Forming Processes in the Solar Neighborhood
Information
Symposium - International Astronomical Union , Volume 115: Star Forming Regions , 1987 , pp. 388 - 390
Copyright
Copyright © Reidel 1987 

References

Kaburaki, O.: 1986 Monthly Notices Roy. Astron. Soc. in press.Google Scholar
Mundt, R., and Friend, J.W.: 1983, Astrophys. J. 274, L83.Google Scholar
Mundt, R., Stocke, J., and Stockman, H.S.: 1983, Astrophys. J. 265, L71.Google Scholar
Rodríguez, L.F.: 1987, this volume.Google Scholar
Strom, S.E.: 1987, this volume.Google Scholar