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Exploring Galactic open clusters with Gaia. II. Dynamical Evolution and Stellar Population Properties in Fifteen Nearby Open Clusters
J Alfonso, A García-Varela, K Vieira - Publications of the …, 2026 - iopscience.iop.org
… masses for single stars are derived from a cubic spline relation with G-band magnitude, while binary component masses are estimated via a simulation-based inference …
Link to paper
… masses for single stars are derived from a cubic spline relation with G-band magnitude, while binary component masses are estimated via a simulation-based inference …