Stellar-opacity calculations, 2: Lecture 3

Details Stellar-opacity calculations, 2: Lecture 3 Stellar-opacity calculations, 2: Lecture 3

Mar 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983stin...8333807c&link_type=abstract

Presented at the Swiss Society of Astrophysics and Astromony Conf., Saas Fee, Switzerland, 21-26 Mar. 1983

Astronomy and Astrophysics

Astrophysics

Absorption Spectra, Atomic Spectra, Molecular Spectra, Opacity, Spectral Bands, Stellar Evolution, Stellar Spectra, Chemical Composition, Ionization, Molecules, Stellar Structure

Scientific paper

The effects on opacities of atomic lines and molecular bands are
discussed. It was the realization that these atomic lines were important
for the opacity and the radiation flow in stars that allowed the field
of stellar evolution to greatly flower in the 1960's and 1970's. Our
understanding of stellar structure and evolution is now very deep.

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