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Polynomial partition function approximations of 344 atomic and molecular species
The Astrophysical Journal Supplement Series1981Vol. 45, pp. 621–621
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Abstract
Approximations of 344 atomic and molecular partition functions are given for a temperature range from 1000 to 16000 K. These approximations are useful for the calculation of the equation of state and the line and continuum opacity of intermediate and late-type stellar atmospheres.
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