Figure 2 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 2.

Our sample shown in an H-R-Diagram, based on the ﹩{T}_{\mathrm{eff}}﹩ and ﹩\mathrm{log}\,g﹩ determined from the LIKC/APF spectra (see Table 3). Yale-Yonsei 12 ﹩\mathrm{Gyr}﹩ isochrones with [α/Fe] = +0.4 and [Fe/H] = −2.5, −3.0, and −3.5 from Demarque et al. (2004) overplotted as reference.

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