Fig. 9
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Comparison of MW SFHs from literature. The SFH of the solar neighbourhood derived in this work (black line) compared to Left: the SFH of Ruiz-Lara et al. (2020); Mor et al. (2019); del Alcázar-Julià et al. (2025) determined by CMD fitting of stars located in the solar neighbourhood and middle: the chemical evolution models of Spitoni et al. (2024); Chen & Prantzos (2025). Right: SFR of the inner disc (Rbirth < 10 kpc) compared with the one from Snaith et al. (2015).
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