Stellar-opacity Calculations. II. Lecture 3 PDF Download

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Stellar-opacity Calculations. II. Lecture 3

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We turn to the effects on opacities of atomic lines and molecular bands. 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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