Figure 5 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 5.

Comparison of the spectra of the Ba and Fe lines in BS 16920–017 (filled circles) and HD 4306 (solid line). The Ba line of BS 16920–017 is significantly weaker than that of HD 4306.

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