Figure 3 from Spectroscopic Studies of Extremely Metal-poor Stars with the Subaru High Dispersion Spectrograph. V. The Zn-enhanced Metal-poor Star BS 16920-017

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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 3.

Comparison of the spectra of the Zn lines in BS 16920–017 (filled circles) and HD 4306 (solid line). Although the metallicity of HD 4306 is higher than BS 16920–017, the Zn line is clearly stronger in BS 16920–017.

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