CHEMICAL COMPOSITION AND ATMOSPHERE PARAMETERS OF THE DOUBLE-MODE CEPHEID U TRA

Four high-resolution spectra of the doble-mode Cepheid UTrA have been obtained during its pulsational period. For the first time, we obtained accurate atmosphere parameters and the chemical abundance of a number of elements, in particular of sodium, magnesium, and aluminium. We estimated the mean Teff...

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Main Authors: I. A. Usenko, A. Yu. Knyazev, L. N. Berdnikov, V. V. Kravtsov
Format: Article
Language:English
Published: Odessa I. I. Mechnykov National University 2013-11-01
Series:Odessa Astronomical Publications
Online Access:http://oap.onu.edu.ua/article/view/82357
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author I. A. Usenko
A. Yu. Knyazev
L. N. Berdnikov
V. V. Kravtsov
author_facet I. A. Usenko
A. Yu. Knyazev
L. N. Berdnikov
V. V. Kravtsov
author_sort I. A. Usenko
collection DOAJ
description Four high-resolution spectra of the doble-mode Cepheid UTrA have been obtained during its pulsational period. For the first time, we obtained accurate atmosphere parameters and the chemical abundance of a number of elements, in particular of sodium, magnesium, and aluminium. We estimated the mean Teff =608529K, logg=2.000.15, and Vt =3.900.25kms 1. A deficit of carbon ([C=H] =–0.350.23dex), over abundance of both sodium  ([Na=H]=+0.150.25dex) and aluminium ([Al=H] =+0.300.32dex) are typical for Cepheids passing through the first dredge-upphase. The abundance of iron ([Fe=H]=+0.010.15dex) is very close to the solar one. Moreover, we find that -elements, those of Fe-group, as well as ”light” - and ”heavy”-, s- and r- process elements, all of them have abundances close  to solar values, too, excepting may be severale lements with slight enhance or deficit.
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spelling doaj.art-9fc17f860f244893b96a207549dc12832022-12-21T23:47:25ZengOdessa I. I. Mechnykov National UniversityOdessa Astronomical Publications1810-42152013-11-0126112713010.18524/1810-4215.2013.26.8235782357CHEMICAL COMPOSITION AND ATMOSPHERE PARAMETERS OF THE DOUBLE-MODE CEPHEID U TRAI. A. Usenko0A. Yu. KnyazevL. N. BerdnikovV. V. KravtsovDepartment of Astronomy, Odessa National UniversityFour high-resolution spectra of the doble-mode Cepheid UTrA have been obtained during its pulsational period. For the first time, we obtained accurate atmosphere parameters and the chemical abundance of a number of elements, in particular of sodium, magnesium, and aluminium. We estimated the mean Teff =608529K, logg=2.000.15, and Vt =3.900.25kms 1. A deficit of carbon ([C=H] =–0.350.23dex), over abundance of both sodium  ([Na=H]=+0.150.25dex) and aluminium ([Al=H] =+0.300.32dex) are typical for Cepheids passing through the first dredge-upphase. The abundance of iron ([Fe=H]=+0.010.15dex) is very close to the solar one. Moreover, we find that -elements, those of Fe-group, as well as ”light” - and ”heavy”-, s- and r- process elements, all of them have abundances close  to solar values, too, excepting may be severale lements with slight enhance or deficit.http://oap.onu.edu.ua/article/view/82357
spellingShingle I. A. Usenko
A. Yu. Knyazev
L. N. Berdnikov
V. V. Kravtsov
CHEMICAL COMPOSITION AND ATMOSPHERE PARAMETERS OF THE DOUBLE-MODE CEPHEID U TRA
Odessa Astronomical Publications
title CHEMICAL COMPOSITION AND ATMOSPHERE PARAMETERS OF THE DOUBLE-MODE CEPHEID U TRA
title_full CHEMICAL COMPOSITION AND ATMOSPHERE PARAMETERS OF THE DOUBLE-MODE CEPHEID U TRA
title_fullStr CHEMICAL COMPOSITION AND ATMOSPHERE PARAMETERS OF THE DOUBLE-MODE CEPHEID U TRA
title_full_unstemmed CHEMICAL COMPOSITION AND ATMOSPHERE PARAMETERS OF THE DOUBLE-MODE CEPHEID U TRA
title_short CHEMICAL COMPOSITION AND ATMOSPHERE PARAMETERS OF THE DOUBLE-MODE CEPHEID U TRA
title_sort chemical composition and atmosphere parameters of the double mode cepheid u tra
url http://oap.onu.edu.ua/article/view/82357
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AT lnberdnikov chemicalcompositionandatmosphereparametersofthedoublemodecepheidutra
AT vvkravtsov chemicalcompositionandatmosphereparametersofthedoublemodecepheidutra