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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 5.

Portions of the Lick/APF spectrum of HD 2796 (shown as blue filled circles) near the lines of Eu II at 4129 Å (top left), Ba II at 6141 Å (top right), Sr II at 4077 Å (bottom left), and Zr II at 4161 Å (bottom right). Best-fit synthetic spectra are also shown (yellow solid line), together with abundance variations (magenta dashed line and cyan dashed–dotted line) of ±0.1 dex (for Eu), ±0.1 dex (for Ba), ±0.3 dex (for Sr), and ±0.5 dex (for Zr).

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