MgH lines in the spectrum of Arcturus

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dc.contributor.authorKushniruk, I.O.
dc.contributor.authorPavlenko, Ya.V.
dc.contributor.authorKaminskiy, B.M.
dc.date.accessioned2017-06-06T19:04:32Z
dc.date.available2017-06-06T19:04:32Z
dc.date.issued2013
dc.description.abstractThe synthetic spectra of MgH lines were computed for the grid of the model atmospheres and compared with the observed spectrum of Arcturus. The parameters of the atmosphere of Arcturus for log g = 1.5 and Tₑff = 4300K were via minimization of deviation between observed and computed spectra and compared with the results of other studies.uk_UA
dc.description.sponsorshipWe thank to Profs. Hinkle, Kurucz, and VALD team for providing databases of astrophysical data used in our work, Oleksiy Ivanyuk and Larisa Yakovina for the helpful comments, and anonymous Referee for some positive remarks.uk_UA
dc.identifier.citationMgH lines in the spectrum of Arcturus / I.O. Kushniruk, Ya.V. Pavlenko, B.M. Kaminskiy // Advances in Astronomy and Space Physics. — 2013. — Т. 3., вип. 1. — С. 29-31. — Бібліогр.: 12 назв. — англ.uk_UA
dc.identifier.issn2227-1481
dc.identifier.urihttps://nasplib.isofts.kiev.ua/handle/123456789/119418
dc.language.isoenuk_UA
dc.publisherГоловна астрономічна обсерваторія НАН Україниuk_UA
dc.relation.ispartofAdvances in Astronomy and Space Physics
dc.statuspublished earlieruk_UA
dc.titleMgH lines in the spectrum of Arcturusuk_UA
dc.typeArticleuk_UA

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Advances in Astronomy and Space Physics, 2013, вип. 1