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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

Jun Fukue
Jun Fukue*
Affiliation:
Astronomical Institute, Osaka Kyoiku University, Japan

Extract

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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 

References

Fukue, J.: 1982, Publ. Astron. Soc. Japan 34, 163.Google Scholar
Fukue, J.: 1983, Publ. Astron. Soc. Japan 35, 539.Google Scholar
Fukue, J., and Yamamoto, S.: 1986, Publ. Astron. Soc. Japan 38, No. 6, in press.Google Scholar