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Wavelengths for satellite-type lines resulting from 2p 1s electron transitions in iron with vacancies in both the 1s and 2s electron shells were calculated, by means of a screening-constant method, for iron in all states of ionization of the outer electron shells. The line for Fe xv differs by percent from the value determined by means of the Hartree-Fock wave functions.
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William J. Veigele (1970) studied this question.
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