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The Computation of Molecular Abundances and Opacities in the Atmospheres of Late-Type Stars
Published online by Cambridge University Press: 04 August 2017
Abstract
The presence of molecules in cool stellar atmospheres can dominate the opacity. Some calculations have been done with a carbon-rich mixture of C/0=2, and the molecules C2, CN, HCN and C2H2 are major sources of opacity due to their large abundances. New calculations with HCN and C2H2 show they can be important.
- Type
- Stellar Atmospheres
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- Copyright © Reidel 1987