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Metallicity of Pleiades Dwarf

  • Conference paper
Precision Spectroscopy in Astrophysics

Part of the book series: ESO Astrophysics Symposia ((ESO))

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Abstract

The goal of our study is to discuss how planet-hosting stars (PHSs) are born by analyzing the chemical homogeneity in open clusters. We obtained the spectra of 18 A,F,G stars in the Pleiades by the high-resolution spectroscopic observations in last January. Out of the 18 stars, the metallcities of 10 stars were derived, and their mean metallicity was obtained to be [Fe/H]mean = +0.02±0.14dex. This high dispersion may imply the chemical diversity in Pleiades. We report the results of our analysis.

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Author information

Authors and Affiliations

  1. Graduate School of Science and Technology, Kobe University, 1-1 Rokkodai, Nada, Kobe, Hyogo, 657-8501, Japan

    H. Funayama, Y. Itoh, Y. Oasa, E. Toyota & T. Mukai

Authors
  1. H. Funayama
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  2. Y. Itoh
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  3. Y. Oasa
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  4. E. Toyota
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  5. T. Mukai
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Editor information

Editors and Affiliations

  1. Centro de Astrofisica da, Univ. do Porto, Rua das Estrelas, 4150-762, Porto, Portugal

    Nuno C. Santos

  2. European Southern Observatory, Karl-Schwarschild-Str. 2, 85748, Garching, Germany

    Luca Pasquini  & Martino Romaniello  & 

  3. Depto. Fisica, Universidade Aveiro, Campus Universitário de Santiago, 3810, Aveiro, Portugal

    Alexandre C. M. Correia

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© 2008 Springer-Verlag Berlin Heidelberg

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Funayama, H., Itoh, Y., Oasa, Y., Toyota, E., Mukai, T. (2008). Metallicity of Pleiades Dwarf. In: Santos, N.C., Pasquini, L., Correia, A.C.M., Romaniello, M. (eds) Precision Spectroscopy in Astrophysics. ESO Astrophysics Symposia. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-540-75485-5_67

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