{"status":"ok","message-type":"work","message-version":"1.0.0","message":{"indexed":{"date-parts":[[2025,10,12]],"date-time":"2025-10-12T03:24:36Z","timestamp":1760239476477,"version":"build-2065373602"},"reference-count":17,"publisher":"MDPI AG","issue":"4","license":[{"start":{"date-parts":[[2020,11,23]],"date-time":"2020-11-23T00:00:00Z","timestamp":1606089600000},"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>Calculated Stark broadening parameters of singly ionized beryllium spectral lines have been reported. Three spectral series have been studied within semiclassical perturbation theory. The plasma conditions cover temperatures from 2500 to 50,000 K and perturber densities 1011 cm\u22123 and 1013 cm\u22123. The influence of the temperature and the role of the perturbers (electrons, protons and He+ ions) on the Stark width and shift have been discussed. Results could be useful for plasma diagnostics in astrophysics, laboratory, and industrial plasmas.<\/jats:p>","DOI":"10.3390\/data5040106","type":"journal-article","created":{"date-parts":[[2020,11,23]],"date-time":"2020-11-23T08:18:23Z","timestamp":1606119503000},"page":"106","update-policy":"https:\/\/doi.org\/10.3390\/mdpi_crossmark_policy","source":"Crossref","is-referenced-by-count":0,"title":["On the Stark Broadening of Be II Spectral Lines"],"prefix":"10.3390","volume":"5","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":"Sorbonne Universit\u00e9, Observatoire de Paris, Universit\u00e9 PSL, CNRS, LERMA, F-92190 Meudon, France"}],"role":[{"role":"author","vocabulary":"crossref"}]},{"given":"Magdalena","family":"Christova","sequence":"additional","affiliation":[{"name":"Department of Applied Physics, Technical University\u2013Sofia, 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":"Sorbonne Universit\u00e9, Observatoire de Paris, Universit\u00e9 PSL, CNRS, LERMA, F-92190 Meudon, France"}],"role":[{"role":"author","vocabulary":"crossref"}]}],"member":"1968","published-online":{"date-parts":[[2020,11,23]]},"reference":[{"key":"ref_1","doi-asserted-by":"crossref","first-page":"871","DOI":"10.1086\/305649","article-title":"Boron abundances and internal mixing in stars. 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