Berkeley 32 was born in the outer Galactic disk (birth radius ~9.8 kpc) and has migrated inward by ~1 kpc, while internal relaxation has segregated its stars by mass.
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Berkeley 32: A Metal-poor and Dynamically Evolved Open Cluster with Evidence of Radial Migration
Berkeley 32 was born in the outer Galactic disk (birth radius ~9.8 kpc) and has migrated inward by ~1 kpc, while internal relaxation has segregated its stars by mass.