OH and CH continuous opacity in solar and stellar atmospheres

Details OH and CH continuous opacity in solar and stellar atmospheres OH and CH continuous opacity in solar and stellar atmospheres

Nov 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987apj...322..992k&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 322, Nov. 15, 1987, p. 992-998.

Physics

Optics

28

Atmospheric Optics, Opacity, Solar Atmosphere, Stellar Atmospheres, Absorption Cross Sections, Hydroxyl Radicals, Molecular Spectra, Spectral Energy Distribution, Visible Spectrum

Scientific paper

Continuous absorption cross sections of OH and CH have been computed for
the temperature range 1000K to 9000K. 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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