Rosseland mean opacities for variable compositions

Details Rosseland mean opacities for variable compositions Rosseland mean opacities for variable compositions

Dec 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992apj...401..361r&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 401, no. 1, p. 361-366.

Physics

Atomic Physics

115

Atomic Physics, Opacity, Oscillator Strengths, Stellar Models, Hydrogen, Main Sequence Stars, Stellar Composition, Stellar Evolution, Stellar Interiors

Scientific paper

We have undertaken a long-term effort to provide improved Rosseland mean opacity tables. In the present paper we present a method to expand our existing tables to include arbitrary values of hydrogen mass fraction. This task was greatly simplified by showing that there exists a correspondence in the equation of state and opacity for sets of mixtures with the same temperature and electron density, but different mass density and composition. Tables for mixtures of variables hydrogen and metal mass fractions as well as the metal constituents can be readily calculated.

Affiliated with

Also associated with

No associations

Rating

Rosseland mean opacities for variable compositions does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Rosseland mean opacities for variable compositions, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Rosseland mean opacities for variable compositions will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1113307