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The resonance lines of sodium and potassium in brown dwarf spectra

Peach, G; Yurchenko, S; Chubb, K; Baraffe, I; Phillips, M; Tremblin, P; (2020) The resonance lines of sodium and potassium in brown dwarf spectra. Contributions of the Astronomical Observatory Skalnaté Pleso , 50 (1) pp. 193-202. 10.31577/caosp.2020.50.1.193. Green open access

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Abstract

Accurate pressure broadened line profiles of alkali resonance doublets are needed for the modelling of atmospheres of cool stars and for generating their synthetic spectra in the region 400 - 900 nm. When the lines utterly dominate their region of the spectrum, it becomes important to represent the profiles accurately over the whole range from the line centre to the far line wings. In this paper we examine the theories of spectral line shapes that have been used and carry out new calculations of the line shapes for the resonance lines of sodium and potassium broadened by helium.

Type: Article
Title: The resonance lines of sodium and potassium in brown dwarf spectra
Open access status: An open access version is available from UCL Discovery
DOI: 10.31577/caosp.2020.50.1.193
Publisher version: https://doi.org/10.31577/caosp.2020.50.1.193
Language: English
Additional information: Open Access article, under the terms of the Creative Commons Attribution License (CC BY 4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited
Keywords: Spectral line broadening calculations, alkali resonance doublets, cool stars: synthetic spectra
UCL classification: UCL
UCL > Provost and Vice Provost Offices > UCL BEAMS
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Physics and Astronomy
URI: https://discovery-pp.ucl.ac.uk/id/eprint/10094086
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