A precise new method to correcting temperature in stellar atmospheres
Calculations of energy balance in model stellar atmospheres for cold and moderately cold stars show that the overall energy gained or lost at the Lyman frequencies (lines plus continuum) can be up to 20 orders of magnitude higher than in the rest of the spectrum. Due to the great optical depth at those frequencies, however, monochromatic mean
Cardona, O. et al.
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2002