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Berkeley 32: A Metal-poor and Dynamically Evolved Open Cluster with Evidence of Radial Migration

  • Authors: D. C. Çinar, D. Bisht, Ing-Guey Jiang, W. H. Elsanhoury, K. Belwal, Selçuk Bilir

D. C. Çinar et al 2026 The Astronomical Journal 172 .

  • Provider: AAS Journals

Caption: Figure 9.

RCDFs of evolved, MSTO, and MS populations in Berkeley 32. The radial distance corresponds to the projected angular separation from the cluster center in arcminutes. Populations were selected according to their G-band magnitude ranges and membership probabilities.

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