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Article contents
On the Condensation of Interstellar Material
Published online by Cambridge University Press: 03 August 2017
Extract
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