Calculations of the spectral line broadening for 1s2 1S-1snp 1p transitions in helium-like ions have been performed for emitters with relatively high Z (silicon and argon). These calculations illustrate the plasma dependent shifts and asymmetries which are due to the high emitter charge. A discussion of the effects is presented, with particular reference to the deviations from the corresponding hydrogenic line profiles.
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Lee et al. (1979) studied this question.
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