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THE TRANSFER OF RADIATION
PHYSICAL PROPERTIES OF GASES ABSORPTION COEFFICIENTS
10 other sections not shown
absorption abundance approximately assumed atmosphere atoms becomes calculated central Chapter cluster coefficient compared composition computed considered constant continuous contraction convective core corresponding curve density depends depth derived determined diagram discussed distribution effective electron element energy envelope equal equation equilibrium example expressed factor Figure flux fraction frequency function given gives helium hydrogen Iben included increase indicated initial integration intensity interior ionization ions layers lower luminosity magnitude main sequence mass matter mean measured nucleus observed obtained occurs opacity particles present pressure produced quantities radiation radiative radius reactions reference region relation represent shell shown shows solar solution spectral stars stellar surface Table temperature tracks units University of Chicago values variables various wavelength zero