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CHEMICAL COMPOSITION OF INTERMEDIATE-MASS STAR MEMBERS OF THE M6 (NGC 6405) OPEN CLUSTER
2016 The Astronomical Journal 151 49.
Caption: Figure 8.
Abundances of C, O, Mg, and Si relative to the Sun (Grevesse & Sauval 1998) vs. ﹩{T}_{\mathrm{eff}}﹩ and ﹩{v}_{{\rm{e}}}\mathrm{sin}i﹩.
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