Molecular Opacity and Stellar Structure

Details Molecular Opacity and Stellar Structure Molecular Opacity and Stellar Structure

Mar 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992rmxaa..23..217c&link_type=abstract

Revista Mexicana de Astronomia y Astrofisica, 23, 217

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RESUMEN. Se han construfdo modelos para estrellas de baja masa de la Secuencia Principal con nuevas opacidades moleculares. Se encuentra que, a pesar de las diferencias entre las nuevas y las viejas opacidades moleculares, los modelos virtualmente no cambian. Estas circunstancias permiten estimar con mayor facilidad la importancia de otros factores ffsicos en los modelos, tales como la ecuaci6n de estado y la generaci6n de energfa. ABSTRACT. Models of low-mass stars on the Main Sequence have been constructed with the help of new `molecular opacities. It is found that, in spite of the differences between the new and old molecular opacities, the models are virtually unchanged. This circumstance permits more easily the assessment of the importance of other aspects of the physics, such as equation of state and energy generation, used in the modelling. Key words: OPACITIES - STARS: ATMOSPHERES - STARS: LATE-TYPE

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