DC FieldValueLanguage
dc.contributor.authorVučetić, M. M.en
dc.contributor.authorTrčka, Anaen
dc.contributor.authorArbutina, Bojanen
dc.contributor.authorĆiprijanović, Aleksandraen
dc.contributor.authorPavlović, Markoen
dc.contributor.authorUrošević, Draganen
dc.contributor.authorPetrov, Nikolaen
dc.date.accessioned2020-05-01T20:28:56Z-
dc.date.available2020-05-01T20:28:56Z-
dc.date.issued2018-01-01en
dc.identifier.issn10556796en
dc.identifier.urihttp://researchrepository.mi.sanu.ac.rs/handle/123456789/1907-
dc.description.abstract© Cambridge Scientific Publishers. We present observations of a Magellanic-type dwarf irregular galaxy NGC 1156 in narrow band [SII] and Hα filters, carried out in November 2015, with the 2 m RCC telescope at Rozhen National Astronomical Observatory in Bulgaria. Although our observations were with the intention to find new extragalactic supernova remnant can- didates, we were successful in the detection of 59 HII regions. We give luminosity function and size distribution for the detected HII regions. Also, we found that re- lation between Hα luminosity and radius of HII regions in NGC 1156 has the slope of 2:7 ± 0:2 in logarithmic presentation, which is in good agreement with theoretical prediction for ionization-bounded HII regions.en
dc.publisherCambridge Scientific-
dc.relation.ispartofAstronomical and Astrophysical Transactionsen
dc.subjectGalaxies | Individual | NGC1156-HII regionsen
dc.titleOptical observations of NGC 1156 galaxy in narrowband [SII] and Hα filtersen
dc.typeArticleen
dc.identifier.doi10.17184/eac.2051-
dc.identifier.scopus2-s2.0-85067027585en
dc.relation.firstpage379en
dc.relation.lastpage386en
dc.relation.issue4en
dc.relation.volume30en
item.fulltextNo Fulltext-
item.openairetypeArticle-
item.grantfulltextnone-
item.cerifentitytypePublications-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
crisitem.author.orcid0000-0003-1281-7192-
crisitem.author.orcid0000-0003-3607-6704-
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