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On the Condensation of Interstellar Material

Published online by Cambridge University Press:  03 August 2017

E. Schatzman
E. Schatzman*
Affiliation:
Institut d'Astrophysique, Paris, France

Extract

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One seeks the condition of spontaneous collapse of a layer of interstellar matter by the method of marginal stability. The radiation field is included in this treatment of the gas-dynamic properties of the interstellar material. The optical model used is that of Ambartsumian's, which neglects interlocking.

Type
Part IV: Cooling and Condensation of Interstellar Matter
Information
Symposium - International Astronomical Union , Volume 8: Cosmical Gas Dynamics , July 1958 , pp. 1012 - 1014
Copyright
Copyright © American Physical Society 1958 

References

1 Chandrasekhar, S., Radiative Transfer (Oxford University Press, New York, 1950).Google Scholar

2 Spitzer, L. and Savedoff, M., Astrophys. J. 111, 593 (1950).Google Scholar