From 19 to 36 new lines each have been identified in K IV, K V, Ca V and Ca VI. In K IV and Ca V these include singlet and intercombination lines. The presence in the nebulae of lines due to the forbidden ³P-¹D transitions in S I, Cl II, A III, K IV and Ca V is discussed.
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I. S. Bowen (1934) studied this question.
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