Opacities for classical Cepheid models

Details Opacities for classical Cepheid models Opacities for classical Cepheid models

Sep 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990apj...360..221i&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 360, Sept. 1, 1990, p. 221-226.

Statistics

Computation

86

Cepheid Variables, Opacity, Stellar Interiors, Stellar Models, Computational Astrophysics, Periodic Variations, Stellar Physics

Scientific paper

Opacities for a classical Cepheid model assuming a King IVa mixture are presented and compared with previous calculations. A significant enhancement of the opacity is reported when compared to the Los Alamos opacity tables. The enhancement is peaked in a region around 2.6 x 10 to the 5th K and falls off rapidly toward lower or higher temperatures. The increase in opacity is mostly due to an improved treatment of the atomic physics.

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