Figure 6 from Metal-poor Stars Observed with the Automated Planet Finder Telescope. I. Discovery of Five Carbon-enhanced Metal-poor Stars from LAMOST

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Metal-poor Stars Observed with the Automated Planet Finder Telescope. I. Discovery of Five Carbon-enhanced Metal-poor Stars from LAMOST

Authors: Mohammad K. Mardini, Haining Li, Vinicius M. Placco, Sofya Alexeeva, Daniela Carollo, Ali Taani, Iminhaji Ablimit, Liang Wang, and Gang Zhao

2019 The Astrophysical Journal 875 89.

Provider: AAS Journals

Caption: Figure 6.

Abundance comparison between this work and Cayrel et al. (2004; for elements with ﹩Z\leqslant 30﹩) and François et al. (2007; for neutron-capture elements). Excluding Sr abundance, the agreement is highly acceptable. The dashed line refers to Δ = 0, and the dashed–dotted lines refer to Δ = ±0.3 dex.

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