1998/05/15 by Luka Č. Popović, L. C. Popovic, Popovic, L. C. +3
Arts and Humanities · Chemistry · Engineering · Physics and Astronomy · #Astrophysics (astro-ph) #Cultural Heritage Materials Analysis #FOS: Physical sciences #Laser-induced spectroscopy and plasma #Mass Spectrometry Techniques and Applications #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/9805204
3 pages, no figure, to appear in: Proc. of the 26th workshop of the European Working Group on CP stars, eds. P. North, A. Schnell and J. Ziznovsky, Contrib. Astr. Obs. Skalnate Pleso Vol. 27, No 3
arxiv created 1998/05/15 · openalex publication_date 1998/05/15 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/07/28
In order to provide atomic data needed for astrophysical investigations, a set of electron-impact broadening parameters for ionized rare-earth element lines should be calculated. We are going to calculate the electron-impact broadening parameters for more than 50 transitions of ionized rare-earth elements. Taking into account that the spectra of these elements are very complex, for calculation we can use the modified semiempirical approach - MSE or simplified MSE. Also, we can estimate these parameters on the basis of regularities and systematic trends.