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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 7.

Distribution of radial velocities as a function of effective temperature for Berkeley 32 member stars. Points are color coded according to the radial-velocity error (eRV; km s−1). The solid horizontal line indicates the weighted mean cluster radial velocity, while the shaded region represents the corresponding 1σ internal velocity dispersion.

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