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Abundances in the atmosphere of the metal-rich planet-host star HD 77338
Репозиторій DSpace/Manakin
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Abundances in the atmosphere of the metal-rich planet-host star HD 77338
Інший ID:
DOI: 10.17721/2227-1481.4.20-24
Посилання:
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.
Підтримка:
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.
Дата:
2014
Переглядів:
781
Завантажень:
445
Анотація:
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.
