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Abstract

Model calculations for laser action in Hei are carried out, when helium plasma is rapidly cooled by expansion. Results are presented for four transitions, two of which, 31 Srarr21 P 0 (lambda7281) and 31 Drarr21 P 0 (lambda6678), show strong population inversion. Available observational evidence for possible laser action in these two lines in Wolf-Rayet and emission-line stars is summarized and discussed.

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