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The Effect of the Gravity of a Circumstellar Torus on Bipolar Jets
Published online by Cambridge University Press: 04 August 2017
Extract
We examine the hydrodynamical wind-type jet in the funnel formed along a rotational axis of accretion tori surrounding a proto star, taking into account the gravitational field produced by torus-gas (Fukue and Yamamoto, in press, 1986). In the current models (e.g. Fukue 1982, 1983), an astrophysical jet was assumed to be accelerated along the funnel considering only the gravitational field of the central object.
- Type
- I. Star Forming Processes in the Solar Neighborhood
- Information
- Symposium - International Astronomical Union , Volume 115: Star Forming Regions , 1987 , pp. 394 - 395
- Copyright
- Copyright © Reidel 1987