Stark broadening of Fe V spectral lines: 4s–4p transitions

نویسندگان

چکیده

ABSTRACT Using the impact semiclassical perturbation approach, widths and shifts of 4s–4p configuration Fe V spectral line profiles due to collisions with electrons, H+, He+, He2 + ions, have been calculated in physical conditions hot white dwarfs. Energy levels oscillator strengths needed for calculation obtained by using Hartree–Fock method relativistic corrections. The results may be interest not only spectroscopic diagnostics astrophysics, but also laboratory plasmas, technological plasmas. will enter STARK-B data base which is free access a node Virtual Atomic Molecular Data Center – VAMDC.

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ژورنال

عنوان ژورنال: Monthly Notices of the Royal Astronomical Society

سال: 2021

ISSN: ['0035-8711', '1365-8711', '1365-2966']

DOI: https://doi.org/10.1093/mnras/stab917