“…In the máximum, a> = 0, and for a Lorenz profile, #(0) = l/nf, where T is the FWHM of the line; a line may be considered optically thin if fe ra L < 0.05, [25], checking that the valué of the optical depth k m L in this work is not in excess of 0.02; for example 0.019 in 6660.0 Á, 0.015 in the 5608.9 Á or 0.006 in the 5042.6 Á. These valúes are less than the lower limit, confirming which the optical thin hypothesis used to be deemed valid; the Unes studied in this study are not resonant.…”