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Equilibrium and Collapse of Rotating Isothermal Clouds

Published online by Cambridge University Press:  04 August 2017

S. Narita ,
M. Kiguchi ,
S. M. Miyama  and
C. Hayashi
S. Narita
Affiliation:
Dept. of, Electronics, Doshisha U., Kyoto 602, Japan
M. Kiguchi
Affiliation:
Inst. of Science and Tech., Kinki U., Osaka 573, Japan
S. M. Miyama
Affiliation:
Dept. of Physics, Kyoto U., Kyoto 606, Japan
C. Hayashi
Affiliation:
Momoyama Yogoro-cho 1, Fushimi-ku, Kyoto 612, Japan

Extract

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We have performed numerical calculations for both static and dynamic structures of molecular clouds in which stars would be formed. The assumption in our calculations is that a cloud, which is embedded in an external hot and tenuous uniform medium, is isothermal and axisymmetric.

Type
I. Star Forming Processes in the Solar Neighborhood
Information
Symposium - International Astronomical Union , Volume 115: Star Forming Regions , 1987 , pp. 377
Copyright
Copyright © Reidel 1987