Calculation of Transition Frequencies and Line Strengths of Water for Cool Star Opacities

Details Calculation of Transition Frequencies and Line Strengths of Water for Cool Star Opacities Calculation of Transition Frequencies and Line Strengths of Water for Cool Star Opacities

Mar 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992rmxaa..23...63m&link_type=abstract

Revista Mexicana de Astronomia y Astrofisica, 23, 63

Statistics

Computation

3

Scientific paper

RESUMEN. Sc presentan calculos de Ia mol6cula de agna basados en primeros principios y usando diferentes superficics del potencial clectr6nico, como el primer paso en un c6mputo mas exacto de la opacidad del agna en estrellas frfas tales como las enanas M. ABSTRACT. First principles calculations for water, using a number of electronic potential surfaces, are presented as a first step towards the computation of an accurate water opacity for cool stars such as M dwarfs. Key word : MOLECULAR PROCESSES - OPACITIES - STARS: ATMOSPHERES - STARS: LATE-TYPE - STARS: LOW-MASS

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