On the Stark broadening of Y III spectral lines.

Astronomy and Astrophysics – Astronomy

Scientific paper

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Spectral Lines: Stark Broadening, Spectral Lines: Yttrium

Scientific paper

Using a semi-classical approach, the authors have considered electron-,
proton-, and ionized helium-impact line widths and shifts for 32 Y III
multiplets, for perturber densities 1014 -
1019cm-3 and temperatures T = 10,000 - 300,000K.

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