Rosseland mean opacities of stellar atmospheres

Details Rosseland mean opacities of stellar atmospheres Rosseland mean opacities of stellar atmospheres

Sep 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981acasn..22..273j&link_type=abstract

Acta Astronomica Sinica, vol. 22, Sept. 1981, p. 273-278. In Chinese, with abstract in English.

Astronomy and Astrophysics

Astronomy

Atmospheric Chemistry, Molecular Absorption, Opacity, Rayleigh Scattering, Stellar Atmospheres, Thomson Scattering, Abundance, Atmospheric Composition, Atmospheric Scattering, Free Electrons, Hydrogen

Scientific paper

Calculations of Rosseland mean opacities in terms of hydrogen particle units are presented for solar type atmospheres. The sources of opacities under consideration include H(-), HI, H2(-), H2(+), He I, He II, C I, C II, C III, N I, N II, N III, O I, O II, Na I, Mg II, Al I, Al II, Si II, Cl I, K I, and Ca II in the absorption form. H I, He I, C I, N I, O I, and H2 were used as sources for Rayleigh scattering, and free electrons were studied in the form of Thomson scattering.

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