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Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/121
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dc.contributor.authorJevremović, D.en_US
dc.contributor.authorDimitrijević, M. S.en_US
dc.contributor.authorPopović, L. Čen_US
dc.contributor.authorDačić, M.en_US
dc.contributor.authorProtić Benišek, V.en_US
dc.contributor.authorBon, E.en_US
dc.contributor.authorGavrilović, N.en_US
dc.contributor.authorKovačević, J.en_US
dc.contributor.authorBenišek, V.en_US
dc.contributor.authorKovačević, Anđelkaen_US
dc.contributor.authorIlić, Draganaen_US
dc.contributor.authorSahal-Bréchot, S.en_US
dc.contributor.authorTsvetkova, K.en_US
dc.contributor.authorSimić, Z.en_US
dc.contributor.authorMalović, M.en_US
dc.date.accessioned2022-08-06T15:18:36Z-
dc.date.available2022-08-06T15:18:36Z-
dc.date.issued2009-07-01-
dc.identifier.issn13876473en
dc.identifier.urihttps://research.matf.bg.ac.rs/handle/123456789/121-
dc.description.abstractWe review recent developments in Serbian Virtual Observatory (SerVO) as well as developments surrounding Virtual Atomic and Molecular Data Center. Main components of SerVO are going to be the archive of photographic plates, database of Stark broadening parameters and stellar evolution database. Photographic plates were obtained at Belgrade Observatory from 1936 to 1996. Data for Stark broadening were obtained using semiclassical perturbation and modified semiempirical theories. Stellar evolution database is a mirror of Darthmouth evolution database with improvement and VO compatible outputs. © 2009 Elsevier B.V. All rights reserved.en_US
dc.language.isoenen_US
dc.publisherElsevieren_US
dc.relation.ispartofNew Astronomy Reviewsen_US
dc.subjectAtomic dataen_US
dc.subjectDatabasesen_US
dc.subjectStark broadeningen_US
dc.subjectStars: evolutionen_US
dc.subjectVirtual Observatoryen_US
dc.titleThe project of Serbian Virtual Observatory and data for stellar atmosphere modelingen_US
dc.typeArticleen_US
dc.identifier.doi10.1016/j.newar.2009.09.002-
dc.identifier.scopus2-s2.0-70449535658-
dc.identifier.isi000272763900020-
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/70449535658-
dc.contributor.affiliationAstronomyen_US
dc.contributor.affiliationAstronomyen_US
dc.relation.issn1387-6473en_US
dc.description.rankM22en_US
dc.relation.firstpage222en_US
dc.relation.lastpage226en_US
dc.relation.volume53en_US
dc.relation.issue7-10en_US
item.openairetypeArticle-
item.cerifentitytypePublications-
item.languageiso639-1en-
item.grantfulltextnone-
item.fulltextNo Fulltext-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
crisitem.author.deptAstronomy-
crisitem.author.deptAstronomy-
crisitem.author.orcid0000-0001-5139-1978-
crisitem.author.orcid0000-0002-1134-4015-
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