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Oxygen Abundances in Metal‐poor Stars

  • Authors: Jon. P. Fulbright and Jennifer A. Johnson

Fulbright & Johnson 2003 The Astrophysical Journal 595 1154.

  • Provider: AAS Journals

Caption: Fig. 15.

Plot of the ﹩\mathrm{log}\,T_{\mathrm{eff}\,}﹩–﹩\mathrm{log}\,g﹩ plane for the three parameter scales analyzed here. The lines are 10 Gyr (dotted lines) and 12 Gyr (solid line) VandenBerg et al. (2000) isochrones of [Fe/H﹩] =-2.31﹩, −1.54, and −0.84.

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