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    Are Stars Really Ingesting Their Planets? Examining an Alternative Explanation by Nadine H. Soliman, Philip F. Hopkins

    Published 2025-01-01
    “…Our results show that the distribution of refractory abundance variations (Δ[X/H]) has extended tails, with about 10%–30% of all stars displaying variations around ∼0.1 dex. These variations are comparable to the accretion of 2–5 M _⊕ of planetary material into the convective zones of Sun-like stars. …”
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