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Stark broadening of Y III spectral lines

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Abstract

Using a semiclassical approach, we have considered electron-, proton-, and ionized helium-impact line width and shifts for 32 Y III multiplets.

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Authors and Affiliations

  1. Astronomical Observatory, Volgina 7, 11050, Serbia, Belgrade, Yugoslavia

    M. S. Dimitrijević

  2. Laboratorie “Astrophysique, Atomes et Molécules”, Départment Atomes at Molécules en Astrophysique, Unité associé au C.N.R.S. N 812, Observatoire de Paris-Meudon, 92190, Meudon, France

    S. Sahal-Bréchot

Authors
  1. M. S. Dimitrijević
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  2. S. Sahal-Bréchot
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Additional information

Published in Zhurnal Prikladnoi Spektroskopii, Vol. 65, No. 4, pp. 476–481, July–August, 1998.

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Dimitrijević, M.S., Sahal-Bréchot, S. Stark broadening of Y III spectral lines. J Appl Spectrosc 65, 492–498 (1998). https://doi.org/10.1007/BF02675637

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  • DOI: https://doi.org/10.1007/BF02675637

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