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Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/2996
DC FieldValueLanguage
dc.contributor.authorPopović, Luka Čen_US
dc.contributor.authorStavrev, K Yen_US
dc.contributor.authorTsvetkova, Ken_US
dc.contributor.authorTsvetkov, Men_US
dc.contributor.authorIlić, Draganaen_US
dc.contributor.authorSanchez, S Fen_US
dc.contributor.authorRichter, G Men_US
dc.date.accessioned2025-12-12T16:38:02Z-
dc.date.available2025-12-12T16:38:02Z-
dc.date.issued2005-
dc.identifier.urihttps://research.matf.bg.ac.rs/handle/123456789/2996-
dc.description.abstractThe Sy 1 galaxy Mrk 1040 and its close companion LEDA 212995 have been observed in several narrow spectral bands, as well as in the U and I bands, in order to look for possible interaction between them. The analysis of the observations shows a very strong point-like innermost center of Mrk 1040 that is from AGN, an irregular structure of the companion expected in the case of a star-forming region, and different star-forming regions in the stellar disk of Mrk 1040. No tidal tail of young stars between Mrk 1040 and LEDA 212995 has been identified.en_US
dc.language.isoenen_US
dc.publisherBulgarian Academy of Sciencesen_US
dc.relation.ispartofAerospace Research in Bulgariaen_US
dc.titleMrk 1040 and its companion LEDA 212995en_US
dc.typeArticleen_US
dc.contributor.affiliationAstronomyen_US
dc.relation.issn1313-0927en_US
dc.relation.firstpage126en_US
dc.relation.lastpage130en_US
dc.relation.volume20en_US
item.openairetypeArticle-
item.languageiso639-1en-
item.grantfulltextnone-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextNo Fulltext-
item.cerifentitytypePublications-
crisitem.author.deptAstronomy-
crisitem.author.orcid0000-0002-1134-4015-
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