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Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/275
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dc.contributor.authorVučetić, M. M.en_US
dc.contributor.authorArbutina, Bojanen_US
dc.contributor.authorUrošević, Dejanen_US
dc.date.accessioned2022-08-06T17:48:11Z-
dc.date.available2022-08-06T17:48:11Z-
dc.date.issued2015-01-01-
dc.identifier.issn00358711en
dc.identifier.urihttps://research.matf.bg.ac.rs/handle/123456789/275-
dc.description.abstractIn this paper, we present the most up-to-date list of nearby galaxies with optically detected supernova remnants (SNRs). We discuss the contribution of the Hα flux from the SNRs to the total Hα flux and its influence on the derived star formation rate (SFR) for 18 galaxies in our sample. We found that the contribution of SNR flux to the total Hα flux is 5 ± 5 per cent. Due to the observational selection effects, the SNR contamination of SFRs derived herein represents only a lower limit.en
dc.relation.ispartofMonthly Notices of the Royal Astronomical Societyen
dc.subjectGalaxies: ISMen
dc.subjectGalaxies: star formationen
dc.subjectISM: supernova remnantsen
dc.subjectStars: formationen
dc.titleOptical supernova remnants in nearby galaxies and their influence on star formation rates derived from Hα emissionen_US
dc.typeArticleen_US
dc.identifier.doi10.1093/mnras/stu2093-
dc.identifier.scopus2-s2.0-84924439642-
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/84924439642-
dc.contributor.affiliationAstronomyen_US
dc.contributor.affiliationAstronomyen_US
dc.relation.firstpage943en
dc.relation.lastpage958en
dc.relation.volume446en
dc.relation.issue1en
item.fulltextNo Fulltext-
item.openairetypeArticle-
item.grantfulltextnone-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.cerifentitytypePublications-
crisitem.author.deptAstronomy-
crisitem.author.deptAstronomy-
crisitem.author.orcid0000-0002-8036-4132-
crisitem.author.orcid0000-0003-0665-0939-
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