Please use this identifier to cite or link to this item: https://physrep.ff.bg.ac.rs/handle/123456789/620
DC FieldValueLanguage
dc.contributor.authorMilosavljević, Vladimiren
dc.contributor.authorDimitrijević, M. S.en
dc.contributor.authorDjeniže, S.en
dc.date.accessioned2022-07-12T16:01:43Z-
dc.date.available2022-07-12T16:01:43Z-
dc.date.issued2001-01-01en
dc.identifier.issn0067-0049en
dc.identifier.urihttps://physrep.ff.bg.ac.rs/handle/123456789/620-
dc.description.abstractStark widths of 42 single (Ne II), 10 double (Ne III), and five triple-charged (Ne IV) neon ion spectral lines, interesting for astrophysics, have been measured in a linear low-pressure pulsed arc at electron temperatures of 31,000 and 34,500 K and electron densities of 0.95 × 10 23 and 1.83 × 10 23 m -3 . The measured width values have been compared with the theoretical data calculated by us using semiclassical perturbation formalism. Our measured and calculated Stark width values have also been compared with existing experimental and theoretical data.en
dc.relation.ispartofAstrophysical Journal, Supplement Seriesen
dc.subjectAtomic dataen
dc.subjectLine: profilesen
dc.subjectMethods: laboratoryen
dc.subjectPlasmasen
dc.titleStark widths of the Ne II, Ne III, and Ne IV spectral linesen
dc.typeArticleen
dc.identifier.doi10.1086/321774en
dc.identifier.scopus2-s2.0-0001153658en
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/0001153658en
dc.relation.issue1en
dc.relation.volume135en
dc.relation.firstpage115en
dc.relation.lastpage124en
item.openairetypeArticle-
item.cerifentitytypePublications-
item.fulltextNo Fulltext-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.grantfulltextnone-
crisitem.author.orcid0000-0002-7805-5189-
Appears in Collections:Journal Article
Show simple item record

SCOPUSTM   
Citations

22
checked on Nov 19, 2024

Page view(s)

14
checked on Nov 22, 2024

Google ScholarTM

Check

Altmetric

Altmetric


Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.