Si/-/ opacity

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Apr 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978mnras.183..257j&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 183, Apr. 1978, p. 257-264. Research supported by the Science Research

Astronomy and Astrophysics

Astronomy

2

Absorptivity, Anions, Opacity, Silicon, Stellar Atmospheres, A Stars, Absorption Spectra, B Stars, Electron Transitions, Photodetachment

Scientific paper

The continuous absorption coefficient of Si(-) is calculated from
quantum mechanically determined free-free cross-sections and
experimental photodetachment data. The results indicate that, apart from
hydrogen-deficient late-type stars, Si(-) is a minor source of opacity
in stellar atmospheres.

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