Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/111
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dc.contributor.authorPopović, L. Čen_US
dc.contributor.authorMediavilla, E. G.en_US
dc.contributor.authorBon, E.en_US
dc.contributor.authorIlić, Draganaen_US
dc.contributor.authorRichter, G.en_US
dc.date.accessioned2022-08-06T15:18:35Z-
dc.date.available2022-08-06T15:18:35Z-
dc.date.issued2004-01-01-
dc.identifier.issn00046337en
dc.identifier.urihttps://research.matf.bg.ac.rs/handle/123456789/111-
dc.description.abstractWe present here new spectroscopic observations of Mrk 1040 and LEDA 212995 (Mrk 1040 companion) obtained with the Isaac Newton Telescope (INT). The intensity ratios and widths for the narrow emission lines found in LEDA 212995 are typical of HII regions. The red-shift (0.0169±0.00015) of the object derived from these emission lines is very close to the red-shift of Mrk 1040 (z=0.01665). The weak narrow and broad absorption lines were detected in the Hα wavelength band of LEDA 212995 spectra. These absorptions indicate that the companion might be at least partly obscured by Mrk 1040. Using this and previous observations we discuss the possible physical relationship between these two galaxies.en
dc.relation.ispartofAstronomische Nachrichtenen
dc.subjectGalaxies: Seyferten
dc.subjectLines: profileen
dc.titleH II emission line region in LEDA 212995, a small neighboring galaxy of Mrk 1040en_US
dc.typeArticleen_US
dc.identifier.doi10.1002/asna.200310236-
dc.identifier.scopus2-s2.0-4644363040-
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/4644363040-
dc.contributor.affiliationAstronomyen_US
dc.relation.firstpage376en
dc.relation.lastpage379en
dc.relation.volume325en
dc.relation.issue5en
item.fulltextNo Fulltext-
item.openairetypeArticle-
item.grantfulltextnone-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.cerifentitytypePublications-
crisitem.author.deptAstronomy-
crisitem.author.orcid0000-0002-1134-4015-
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