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Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/2119
DC FieldValueLanguage
dc.contributor.authorŽivadinović, Lazaren_US
dc.contributor.authorMilošević, Stanislaven_US
dc.contributor.authorMilić, Damnjanen_US
dc.date.accessioned2025-07-07T17:22:41Z-
dc.date.available2025-07-07T17:22:41Z-
dc.date.issued2018-
dc.identifier.urihttps://research.matf.bg.ac.rs/handle/123456789/2119-
dc.language.isoenen_US
dc.publisherBeograd : Astronomska observatorijaen_US
dc.relation.ispartofPublications of Astronomical Observatory of Belgradeen_US
dc.titleDensity Profile of the Milky Way: Comparison of Dynamical Model and Monte Carlo Method for Determining Stellar Space Densitiesen_US
dc.typeConference Objecten_US
dc.relation.conferenceSerbian Astronomical Conference (18 ; 2017 ; Belgrade)en_US
dc.relation.publicationProceedings of the XVIII Serbian Astronomical conference, October 17-21, 2017., Belgradeen_US
dc.identifier.doihttp://publications.aob.rs/98/pdf/257-262.pdf-
dc.contributor.affiliationAstronomyen_US
dc.relation.isbn978-86-80019-87-1en_US
dc.relation.issn0373-3742en_US
dc.description.rankM63en_US
dc.relation.firstpage257en_US
dc.relation.lastpage262en_US
dc.relation.volume98en_US
item.languageiso639-1en-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextNo Fulltext-
item.grantfulltextnone-
item.openairetypeConference Object-
item.cerifentitytypePublications-
crisitem.author.deptAstronomy-
crisitem.author.orcid0009-0006-2058-5132-
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