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- W2045976483 abstract "The fluorescent spectra of the Cs principal series lines 4555 and 4593 AA (72P32,1/2/-62S12/) broadened by Kr and Xe were measured up to perturber gas densities of about 4.9*1019 cm-3. In addition, the absorption spectra of the Cs principal series line 3876 AA (62S12/-82P32/) broadened by Xe (1.63*1018<or=NX3<or=1.9*1019 cm-3) were investigated. The existence of secondary satellites was established. The intensity dependence of the quasistatic wings is discussed and qualitatively explained by competitive additive two- and three-body interactions." @default.
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- W2045976483 date "1980-05-14" @default.
- W2045976483 modified "2023-10-18" @default.
- W2045976483 title "Investigation on three-body Cs-noble-gas interaction and secondary satellites" @default.
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- W2045976483 doi "https://doi.org/10.1088/0022-3700/13/9/011" @default.
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