Abstract
We have studied high-resolution SWP spectra of AE Aur andθ2 Ori A, obtained from the International Ultraviolet Explorer Satellite; and derived curve of growth and column densities ofCii,Cii*, Alii, Siii, Siii*,Sii, Crii, Feii, Niii, and Znii. It has been possible to fit these ions on one empirical curve of growth with a velocity parameterb=13 km s−1 for both stars.
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