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dc.creatorDimitrijević, Milan S.
dc.creatorSimić, Zoran
dc.creatorKovačević, Anđelka
dc.creatorValjarević, Aleksandar
dc.creatorSahal-Brechot, Sylvie
dc.date.accessioned2021-09-24T15:33:13Z
dc.date.available2021-09-24T15:33:13Z
dc.date.issued2015
dc.identifier.issn0250-6335
dc.identifier.urihttps://gery.gef.bg.ac.rs/handle/123456789/726
dc.description.abstractIn order to complete Stark broadening data for Ne I spectral lines which are needed for analysis of stellar atmospheres, collisional widths and shifts (the so-called Stark broadening parameters) of 29 isolated spectral lines of neutral neon have been determined within the impact semiclassical perturbation method. Calculations have been performed for the broadening by collisions with electrons, protons and ionized helium for astrophysical applications, and for collisions with ionized neon and argon for laboratory plasma diagnostics. The shifts have been compared with existing experimental values. The obtained data will be included in the STARK-B database, which is a part of the Virtual Atomic and Molecular Data Center - VAMDC.en
dc.publisherIndian Acad Sciences, Bangalore
dc.relationinfo:eu-repo/grantAgreement/MESTD/Basic Research (BR or ON)/176002/RS//
dc.relationParis Observatory
dc.relationCentre National de la Recherche Scientifique (CNRS) - European Commission
dc.relationPNPS (Programme National de Physique Stellaire, INSU-CNRS)
dc.rightsrestrictedAccess
dc.sourceJournal of Astrophysics and Astronomy
dc.subjectStark broadeningen
dc.subjectatomic dataen
dc.subjectNe I: line profilesen
dc.titleStark Widths of Spectral Lines of Neutral Neonen
dc.typeconferenceObject
dc.rights.licenseARR
dcterms.abstractСимић, Зоран; Сахал-Брецхот, Сyлвие; Ковачевић, Aнђелка; Димитријевић, Милан С.; Ваљаревић, Aлександар;
dc.citation.volume36
dc.citation.issue4
dc.citation.spage643
dc.citation.epage659
dc.citation.other36(4): 643-659
dc.citation.rankM23
dc.identifier.wos000368698700020
dc.identifier.doi10.1007/s12036-015-9343-z
dc.identifier.scopus2-s2.0-84956687682
dc.identifier.rcubhttps://hdl.handle.net/21.15107/rcub_gery_726
dc.type.versionpublishedVersion


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