Chemical composition of the RS CVn-type star 29 Draconis

dc.bibliographicCitation.firstPage157eng
dc.bibliographicCitation.issue3-4eng
dc.bibliographicCitation.journalTitleBaltic Astronomyeng
dc.bibliographicCitation.lastPage167eng
dc.bibliographicCitation.volume19
dc.contributor.authorBarisevičius, G.
dc.contributor.authorTautvaišiené, Gražina G.
dc.contributor.authorBerdyugina, Svetlana V.
dc.contributor.authorChorniy, Yuriy
dc.contributor.authorIlyin, Ilya V.
dc.date.accessioned2018-04-25T03:23:28Z
dc.date.available2019-06-28T12:39:41Z
dc.date.issued2010
dc.description.abstractAbundances of 22 chemical elements, including the key elements and isotopes such as 12C, 13C, N and O, are investigated in the spectrum of 33 Psc, a single-lined RS CVn-type binary of low magnetic activity. The high resolution spectra were observed on the Nordic Optical Telescope and analyzed with the MARCS model atmospheres. The following main parameters have been determined: Teff = 4750 K, log g = 2.8, [Fe/H] = -0.09, [C/Fe] = -0.04, [N/Fe] = 0.23, [O/Fe] = 0.05, C/N = 2.14, 12C/13C = 30, which show the first-dredge-up mixing signatures and no extra-mixing.eng
dc.description.versionpublishedVersioneng
dc.formatapplication/pdf
dc.identifier.urihttps://doi.org/10.34657/1429
dc.identifier.urihttps://oa.tib.eu/renate/handle/123456789/4327
dc.language.isoengeng
dc.publisherBerlin : de Gruytereng
dc.relation.doihttps://doi.org/10.1515/astro-2017-0419
dc.rights.licenseCC BY-NC-ND 4.0 Unportedeng
dc.rights.urihttps://creativecommons.org/licenses/by-nc-nd/4.0/eng
dc.subject.ddc530eng
dc.subject.otherstars: RS CVn binarieseng
dc.subject.otherabundances – stars: individual (33 Psc = HD 28)eng
dc.titleChemical composition of the RS CVn-type star 29 Draconiseng
dc.typeArticleeng
dc.typeTexteng
tib.accessRightsopenAccesseng
wgl.contributorKISeng
wgl.contributorAIPeng
wgl.subjectPhysikeng
wgl.typeZeitschriftenartikeleng
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