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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

Christopher M. Sharp
Christopher M. Sharp*
Affiliation:
T-4 Los Alamos National Laboratory, Los Alamos, NM 87545 USA

Abstract

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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
Information
Symposium - International Astronomical Union , Volume 120: Astrochemistry , 1987 , pp. 407 - 408
Copyright
Copyright © Reidel 1987 

References

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Sharp, C.M., , University of St. Andrews (1981).Google Scholar