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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 1.

Comparison of the equivalent widths of HD 2796, the blue circles represent the comparison of this work and Cayrel et al. (2004), while the black triangles represent the comparison of this this work and Li et al. (2015). Note that the biggest discrepancies between our EWs and the literature data are for the strongest lines. Thus, the spectrum-synthesis approach has been used for these lines (e.g., Mg I triplets).

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