{"status":"ok","message-type":"work","message-version":"1.0.0","message":{"indexed":{"date-parts":[[2025,10,11]],"date-time":"2025-10-11T01:08:41Z","timestamp":1760144921723,"version":"build-2065373602"},"reference-count":20,"publisher":"MDPI AG","issue":"6","license":[{"start":{"date-parts":[[2024,5,29]],"date-time":"2024-05-29T00:00:00Z","timestamp":1716940800000},"content-version":"vor","delay-in-days":0,"URL":"https:\/\/creativecommons.org\/licenses\/by\/4.0\/"}],"content-domain":{"domain":[],"crossmark-restriction":false},"short-container-title":["Data"],"abstract":"<jats:p>Data on Stark broadening parameters, spectral line widths, and shifts for 15 multiplets of N VI, whose spectral lines are broadened by collisions with electrons, protons, alpha particles (He III) and B III, B IV, B V and B VI ions, are presented. They have been calculated using the semiclassical perturbation theory, for temperatures from 50,000 K to 2,000,000 K, and perturber densities from 1016 cm\u22123 up to 1024 cm\u22123. The data for e, p and He III are of particular interest for the analysis and modelling of atmospheres of hot and dense stars, as, e.g., white dwarfs, and for investigation of their spectra, and data for boron ions are used for analysis and modelling of laser-driven plasma in proton\u2013boron fusion research.<\/jats:p>","DOI":"10.3390\/data9060077","type":"journal-article","created":{"date-parts":[[2024,6,3]],"date-time":"2024-06-03T10:08:38Z","timestamp":1717409318000},"page":"77","update-policy":"https:\/\/doi.org\/10.3390\/mdpi_crossmark_policy","source":"Crossref","is-referenced-by-count":0,"title":["Data on Stark Broadening of N VI Spectral Lines"],"prefix":"10.3390","volume":"9","author":[{"ORCID":"https:\/\/orcid.org\/0000-0001-9138-8642","authenticated-orcid":false,"given":"Milan S.","family":"Dimitrijevi\u0107","sequence":"first","affiliation":[{"name":"Astronomical Observatory, Volgina 7, 11060 Belgrade, Serbia"},{"name":"LERMA (Laboratoire d\u2019Etudes du Rayonnement et de la Mati\u00e8re en Astrophysique et Atmosph\u00e8re) Observatoire de Paris, Universit\u00e9 PSL (Paris Sciences & Lettres), CNRS (Centre National de la Recherche Scientifique), Sorbonne Universit\u00e9, F-92190 Meudon, France"}],"role":[{"role":"author","vocabulary":"crossref"}]},{"ORCID":"https:\/\/orcid.org\/0000-0002-6851-5436","authenticated-orcid":false,"given":"Magdalena D.","family":"Christova","sequence":"additional","affiliation":[{"name":"Department of Applied Physics, Technical University of Sofia, 1000 Sofia, Bulgaria"}],"role":[{"role":"author","vocabulary":"crossref"}]},{"ORCID":"https:\/\/orcid.org\/0000-0002-2348-2044","authenticated-orcid":false,"given":"Sylvie","family":"Sahal-Br\u00e9chot","sequence":"additional","affiliation":[{"name":"LERMA (Laboratoire d\u2019Etudes du Rayonnement et de la Mati\u00e8re en Astrophysique et Atmosph\u00e8re) Observatoire de Paris, Universit\u00e9 PSL (Paris Sciences & Lettres), CNRS (Centre National de la Recherche Scientifique), Sorbonne Universit\u00e9, F-92190 Meudon, France"}],"role":[{"role":"author","vocabulary":"crossref"}]}],"member":"1968","published-online":{"date-parts":[[2024,5,29]]},"reference":[{"key":"ref_1","doi-asserted-by":"crossref","first-page":"565","DOI":"10.1051\/0004-6361:200810738","article-title":"FUSE spectroscopy of the sdOB primary of the post common-envelope binary LB3459 (AADoradus)","volume":"492","author":"Fleig","year":"2008","journal-title":"Astron. 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Beams"},{"key":"ref_8","doi-asserted-by":"crossref","first-page":"225","DOI":"10.3390\/atoms2020225","article-title":"Widths and Shifts of Isolated Lines of Neutral and Ionized Atoms Perturbed by Collisions with Electrons and Ions: An Outline of the Semiclassical Perturbation (SCP) Method and of the Approximations Used for the Calculations","volume":"2","year":"2014","journal-title":"Atoms"},{"key":"ref_9","first-page":"84","article-title":"On the Stark broadening of N VI spectral lines","volume":"53","author":"Christova","year":"2023","journal-title":"Contrib. Astron. Obs. Skalnat\u00e9 Pleso"},{"key":"ref_10","doi-asserted-by":"crossref","unstructured":"Dimitrijevi\u0107, M.S., Christova, M.D., and Sahal-Br\u00e9chot, S. (2023). Stark broadening of N VI spectral lines. 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