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◆ Astronomy and Astrophysics2026-07-31· Physics

Phosphorus abundances and multi-element co-enrichment in nearby FGK stars

Dario Esposito, Giovanni Covone, Donato Giovannelli, Paola Manini, Christian Magliano, Laura Inno, Luca Cacciapuoti, Víctor M. Rivilla, Vito Saggese, Leonardo Testi, Emanuele Cristiano, L. Tonietti

原始摘要(英文原文)· Original abstract
The distribution of bio-essential elements is key to assessing the chemical `fertility' for life in a galactic context. Among these, phosphorus plays a central role in biomolecules, but it is relatively scarce and difficult to measure in stellar spectra. We aim to characterise phosphorus abundances in nearby FGK stars and quantify how P co-varies with other bio-related elements in different Galactic disk populations. We analysed phosphorus abundances for 233 FGK stars in the solar neighbourhood from the Hypatia Catalog. We studied P/Fe as a function of Fe/H and other elemental abundances, separating thin- and thick-disk stars. We used non-parametric tests and bootstrap resampling to derive median trends, confidence intervals, correlation coefficients, and residual correlations at fixed Fe/H . We also investigated molar ratios involving P relevant to planetary mineralogy. We find a P/Fe -- Fe/H trend broadly similar to that of α elements, supporting a dominant origin in core-collapse supernovae, with some deviations that suggest additional nucleosynthetic channels. Phosphorus shows strong positive correlations with several CHNOPS, α, and Fe-peak elements, especially in the thin disk, where stars with higher phosphorus abundances are enriched in multiple bio-essential and rock-forming species. These co-enrichment patterns remain significant in residual analyses at fixed Fe/H , indicating that they are not a trivial by-product of global metallicity. Thin-disk stars also exhibit higher abundances than thick-disk stars for many elements. The molar P/Mg and P/Si ratios of the Sun are representative of the local stellar population, whereas the relatively elevated solar P/O may have favoured phosphorus bioavailability on Earth. Our study provides a systematic and statistically robust view of how P co-varies with other CHNOPS and α elements in the solar neighbourhood. The results reveal a genuine multi-element co-enrichment pattern beyond metallicity effects and support the use of phosphorus as a tracer of the chemical fertility of galactic environments.
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