How the origin of stars in the Galaxy impacts the composition of planetary building blocks

Open Access

Fig. 5

PBB mass fraction distribution of Fe₃O₄ (left panels) and Mg₂Si0₃ (right panels) for T > 150 K (inner proto-planetary disc) in the [α/Fe]–[Fe/H] diagram. We display the surveys APOGEE-DR17 (top panels) and GALAH-DR3 (bottom panels).

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