Bowen, I. S. (1937) The low terms in Cr III, Cr IV, Mn IV and Fe V. Physical Review, 52 (11). pp. 1153-1156. ISSN 0031-899X. http://resolver.caltech.edu/CaltechAUTHORS:BOWpr37c
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Most of the strong lines arising from the d3, d24s and d24p configurations of Cr IV and the d4, d34s and d34p configurations of Cr III, Mn IV and Fe V have been classified. The presence of forbidden lines of these ions in astronomical sources is discussed.
|Additional Information:||©1937 The American Physical Society. Received 4 October 1937.|
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|Deposited By:||Tony Diaz|
|Deposited On:||19 Oct 2006|
|Last Modified:||26 Dec 2012 09:12|
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