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Molecular Abundances in IRC+10216
Published online by Cambridge University Press: 14 August 2015
Abstract
The observed molecular column-densities in IRC +10216 can be matched by chemical-equilibrium calculations for T∼1250°K, P∼100 dyn cm-2 and no graphite grain formation. Condensation of silicon carbide into grains may explain the low observed abundances of SiO and SiS.
- Type
- Research Article
- Information
- Symposium - International Astronomical Union , Volume 87: Interstellar Molecules , 1980 , pp. 497 - 502
- Copyright
- Copyright © Reidel 1980