Abstract

Improved energy levels for V xii, Cr xiii, Mn xiv, and Co xvi are obtained from comparison of observed values with results calculated by the Superstructure program. Predicted wavelengths of important intercombination lines are given and some probable misidentifications in the literature are noted.

© 1979 Optical Society of America

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Corrections

S. O. Kastner and A. K. Bhatia, "Errata," J. Opt. Soc. Am. 70, 893-893 (1980)
https://www.osapublishing.org/josa/abstract.cfm?uri=josa-70-7-893

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