Abundances in the atmosphere of the metal-rich planet-host star HD 77338

Abundances of Fe, Si, Ni, Ti, Na, Mg, Cu, Zn, Mn, Cr and Ca in the atmosphere of the K-dwarf HD 77338 are determined and discussed. HD 77338 hosts a hot Uranus-like planet and is currently the most metal-rich single star to host any planet. Determination of abundances was carried out in the framewor...

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Опубліковано в: :Advances in Astronomy and Space Physics
Дата:2014
Автори: Kushniruk, I.O., Pavlenko, Ya.V., Jenkins, J.S., Jones, H.R.A.
Формат: Стаття
Мова:English
Опубліковано: Головна астрономічна обсерваторія НАН України 2014
Онлайн доступ:https://nasplib.isofts.kiev.ua/handle/123456789/119803
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Назва журналу:Digital Library of Periodicals of National Academy of Sciences of Ukraine
Цитувати:Abundances in the atmosphere of the metal-rich planet-host star HD 77338 / I.O. Kushniruk, Ya.V. Pavlenko, J.S. Jenkins, H.R.A. Jones // Advances in Astronomy and Space Physics. — 2014. — Т. 4., вип. 1-2. — С. 20-24. — Бібліогр.: 20 назв. — англ.

Репозитарії

Digital Library of Periodicals of National Academy of Sciences of Ukraine
id nasplib_isofts_kiev_ua-123456789-119803
record_format dspace
spelling Kushniruk, I.O.
Pavlenko, Ya.V.
Jenkins, J.S.
Jones, H.R.A.
2017-06-09T19:35:13Z
2017-06-09T19:35:13Z
2014
Abundances in the atmosphere of the metal-rich planet-host star HD 77338 / I.O. Kushniruk, Ya.V. Pavlenko, J.S. Jenkins, H.R.A. Jones // Advances in Astronomy and Space Physics. — 2014. — Т. 4., вип. 1-2. — С. 20-24. — Бібліогр.: 20 назв. — англ.
2227-1481
DOI: 10.17721/2227-1481.4.20-24
https://nasplib.isofts.kiev.ua/handle/123456789/119803
Abundances of Fe, Si, Ni, Ti, Na, Mg, Cu, Zn, Mn, Cr and Ca in the atmosphere of the K-dwarf HD 77338 are determined and discussed. HD 77338 hosts a hot Uranus-like planet and is currently the most metal-rich single star to host any planet. Determination of abundances was carried out in the framework of a self-consistent approach developed by Pavlenko et al. (2012). Abundances were computed iteratively by the ABEL8 code, and the process converged after 4 iterations. We find that most elements follow the iron abundance, however some of the iron peak elements are found to be over-abundant in this star.
JSJ acknowledges the support of the Basal-CATA grant. YP's work has been supported by an FP7 POSTAGBinGALAXIES grant (No. 269193; International Research Staff Exchange Scheme). Authors thank the compilers of the international databases used in our study: SIMBAD (France, Strasbourg), VALD (Austria, Vienna), and the authors of the atlas of the spectrum of the Sun as a star. We thank the anonymous Referee for some reasonable remarks 1 and helpful comments.
en
Головна астрономічна обсерваторія НАН України
Advances in Astronomy and Space Physics
Abundances in the atmosphere of the metal-rich planet-host star HD 77338
Article
published earlier
institution Digital Library of Periodicals of National Academy of Sciences of Ukraine
collection DSpace DC
title Abundances in the atmosphere of the metal-rich planet-host star HD 77338
spellingShingle Abundances in the atmosphere of the metal-rich planet-host star HD 77338
Kushniruk, I.O.
Pavlenko, Ya.V.
Jenkins, J.S.
Jones, H.R.A.
title_short Abundances in the atmosphere of the metal-rich planet-host star HD 77338
title_full Abundances in the atmosphere of the metal-rich planet-host star HD 77338
title_fullStr Abundances in the atmosphere of the metal-rich planet-host star HD 77338
title_full_unstemmed Abundances in the atmosphere of the metal-rich planet-host star HD 77338
title_sort abundances in the atmosphere of the metal-rich planet-host star hd 77338
author Kushniruk, I.O.
Pavlenko, Ya.V.
Jenkins, J.S.
Jones, H.R.A.
author_facet Kushniruk, I.O.
Pavlenko, Ya.V.
Jenkins, J.S.
Jones, H.R.A.
publishDate 2014
language English
container_title Advances in Astronomy and Space Physics
publisher Головна астрономічна обсерваторія НАН України
format Article
description Abundances of Fe, Si, Ni, Ti, Na, Mg, Cu, Zn, Mn, Cr and Ca in the atmosphere of the K-dwarf HD 77338 are determined and discussed. HD 77338 hosts a hot Uranus-like planet and is currently the most metal-rich single star to host any planet. Determination of abundances was carried out in the framework of a self-consistent approach developed by Pavlenko et al. (2012). Abundances were computed iteratively by the ABEL8 code, and the process converged after 4 iterations. We find that most elements follow the iron abundance, however some of the iron peak elements are found to be over-abundant in this star.
issn 2227-1481
url https://nasplib.isofts.kiev.ua/handle/123456789/119803
citation_txt Abundances in the atmosphere of the metal-rich planet-host star HD 77338 / I.O. Kushniruk, Ya.V. Pavlenko, J.S. Jenkins, H.R.A. Jones // Advances in Astronomy and Space Physics. — 2014. — Т. 4., вип. 1-2. — С. 20-24. — Бібліогр.: 20 назв. — англ.
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AT joneshra abundancesintheatmosphereofthemetalrichplanethoststarhd77338
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