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On Stark Broadening of Heavy Element Lines in A-Type Star Spectra: Bi II Lines
Published online by Cambridge University Press: 12 April 2016
Abstract
We report here results of Bi II spectral lines Stark broadening research within the modified semiempirical approach. The strong absorption Bi II lines observed in Hg – Mn star atmospheres have been investigated as well as the influence of the departure from LS – coupling and the correct knowledge of ionization potential. The obtained results have been compared with other estimations and with experimental results.
- Type
- I. General Properties of CP Stars
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- Copyright © Astronomical Society of the Pacific 1993