Stark broadening of B I spectral lines-Reference-Cited by-同舟云学术

Stark broadening of B I spectral lines

Published:2021-10-18 Issue:3 Volume:509 Page:3203-3208
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Dimitrijević Milan S¹²³^ORCID,Christova Magdalena D⁴,Sahal-Bréchot Sylvie²

Affiliation:

1. Astronomical Observatory, Volgina 7, 11060 Belgrade, Serbia

2. LERMA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, 5 Place Jules Janssen, 92190 Meudon, France

3. Institute Isaac Newton of Chile, Yugoslavia Branch, 11060 Belgrade, Serbia

4. Department of Applied Physics, Technical University-Sofia, 1000 Sofia, Bulgaria

Abstract

ABSTRACT We calculated widths and shifts due to collisions with electrons, protons, and He II ions for 66 multiplets of neutral boron, using the semiclassical perturbation theory. The range of temperatures is from 2500 to 50 000 K and electron density values are within the range 1011–1019 cm−3. The obtained Stark broadening parameters have been compared to other theoretical and experimental results.

Funder

COST

CNRS

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/advance-article-pdf/doi/10.1093/mnras/stab2975/40718254/stab2975.pdf

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