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Some problems in determining elemental abundances in the atmospheres of giants and dwarfs of the HR 1614 moving cluster

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Abstract

The atmospheric abundances of various chemical elements and other atmospheric parameters of four stars belonging to the HR 1614 moving cluster are determined and analyzed using a single technique. For three of the stars, the derived atmospheric parameters are typical of stars of their types, and their elemental abundances are close to those determined earlier for these and other stars of the moving cluster. However, the atmospheric parameters derived for the red dwarf HD 32147 would be more typical of a giant, and its metallicity is much lower than is characteristic of stars of this moving group.

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Authors and Affiliations

  1. Institute of Astronomy, Russian Academy of Sciences, ul. Pyatnitskaya 48, Moscow, 119017, Russia

    L. I. Antipova & A. A. Boyarchuk

Authors
  1. L. I. Antipova
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  2. A. A. Boyarchuk
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Correspondence to L. I. Antipova.

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Original Russian Text © L.I. Antipova, A.A. Boyarchuk, 2015, published in Astronomicheskii Zhurnal, 2015, Vol. 92, No. 11, pp. 902–906.

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Antipova, L.I., Boyarchuk, A.A. Some problems in determining elemental abundances in the atmospheres of giants and dwarfs of the HR 1614 moving cluster. Astron. Rep. 59, 1015–1018 (2015). https://doi.org/10.1134/S1063772915110013

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  • DOI: https://doi.org/10.1134/S1063772915110013

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