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Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/2829
DC FieldValueLanguage
dc.contributor.authorAnđelić, Milicaen_US
dc.contributor.authorArbutina, Bojanen_US
dc.contributor.authorK., Stavreven_US
dc.contributor.authorUrošević, Dejanen_US
dc.date.accessioned2025-10-29T09:36:31Z-
dc.date.available2025-10-29T09:36:31Z-
dc.date.issued2011-
dc.identifier.urihttps://research.matf.bg.ac.rs/handle/123456789/2829-
dc.description.abstractIn this paper we derived star formation rate for irregular dwarf galaxy Holmberg IX, member of M81 galaxy group. Star formation rate is calculated using Ha fluxes of HII regions in this galaxy, observed in March 2008 from National astronomical observatory Rozhen, Bulgariaen_US
dc.language.isoenen_US
dc.publisherBeograd : Astronomska opservatorijaen_US
dc.titleStar Formation Rate in Holmberg IX Dwarf Galaxyen_US
dc.typeConference Objecten_US
dc.relation.conferenceNational Conference of Astronomers of Serbia (16 ; 2011 ; Belgrade)en_US
dc.relation.publication16th National Conference of Astronomers of Serbia, Book of abstractsen_US
dc.identifier.urlhttp://nkas.aob.rs/AbsBook.pdf-
dc.contributor.affiliationAstronomyen_US
dc.contributor.affiliationAstronomyen_US
dc.contributor.affiliationAstronomyen_US
dc.description.rankM64en_US
dc.relation.firstpage62en_US
dc.relation.lastpage62en_US
item.openairetypeConference Object-
item.fulltextNo Fulltext-
item.languageiso639-1en-
item.cerifentitytypePublications-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.grantfulltextnone-
crisitem.author.deptAstronomy-
crisitem.author.deptAstronomy-
crisitem.author.deptAstronomy-
crisitem.author.orcid0000-0003-3146-234X-
crisitem.author.orcid0000-0002-8036-4132-
crisitem.author.orcid0000-0003-0665-0939-
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