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

Vernadsky National Library of Ukraine

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Поле Співвідношення
 
Title Abundances in the atmosphere of the metal-rich planet-host star HD 77338
 
Creator Kushniruk, I.O.
Pavlenko, Ya.V.
Jenkins, J.S.
Jones, H.R.A.
 
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.
 
Date 2017-06-09T19:35:13Z
2017-06-09T19:35:13Z
2014
 
Type Article
 
Identifier 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
http://dspace.nbuv.gov.ua/handle/123456789/119803
 
Language en
 
Relation Advances in Astronomy and Space Physics
 
Publisher Головна астрономічна обсерваторія НАН України