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Spectroscopic Studies of Extremely Metal-poor Stars with the Subaru High Dispersion Spectrograph. V. The Zn-enhanced Metal-poor Star BS 16920-017

  • Authors: Satoshi Honda, Wako Aoki, Timothy C. Beers, and Masahide Takada-Hidai

Honda et al. 2011 The Astrophysical Journal 730 77.

  • Provider: AAS Journals

Caption: Figure 2.

Upper panel: [Zn/Fe] abundance ratios as a function of [Fe/H] for our sample stars (filled circles). Results of previous studies are shown by open circles (Sneden et al. 1991; Johnson 2002; Mishenina et al. 2002; Ivans et al. 2003; Cayrel et al. 2004; Aoki et al. 2005; Nissen et al. 2007; Saito et al. 2009). Lower panel: the average [Zn/Fe] abundance ratios in 0.2 dex bins of [Fe/H] are shown by large filled circles for our sample and by open circles for those of previous studies. The bar indicates the standard deviation of the [Zn/Fe] values of each bin. The data of BS 16920–017 are not included in the statistics.

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