OH and CH continuous opacity in solar and stellar atmospheres
Continuous absorption cross sections of OH and CH have been computed for the temperature range 1000 K to 9000 K. Both OH and CH produce significant ultraviolet opacity in the sun and cool stars. CH is also significant in the visible at 400 nm.
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Published in | The Astrophysical journal Vol. 322; no. 2; pp. 992 - 998 |
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Main Authors | , , |
Format | Journal Article |
Language | English |
Published |
Legacy CDMS
University of Chicago Press
15.11.1987
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Subjects | |
Online Access | Get full text |
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