The atmospheric lithium abundances of solar analogues of their lithium abundances, the stars (which are located in a narrow range of temperatures of 5650-5900
K) can
Observational Constraints on Potassium Synthesis during the Formation of Stars of the Galactic Disk (log ε ⊙ (
K) = 5.12). As the stellar metallicity increases from [Fe/H] = (-1.0) to (0.2) dex, the [
K Observational Constraints on Potassium Synthesis during the Formation of Stars of the Galactic Disk (log ε ⊙ (
K) = 5.12). As the stellar metallicity increases from [Fe/H] = (-1.0) to (0.2) dex, the [
K