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The intensity profiles of cesium principal series lines and the associated satellite bands produced by moderately high pressures of xenon are calculated on the basis of a Lennard-Jones potential and collision broadening. Experimental measurements of the contours show fairly good agreement, especially for high series members. Intensity ratios of the satellite to the parent line, calculated for binary interactions only, agree with measurements at several different pressures.
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Kielkopf et al. (1970) studied this question.
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