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Photometry of the Four Anti-Galactocentric Old Open Clusters: Czernik 30, Berkeley 34, Berkeley 75, and Berkeley 76

  • Authors: Hyobin Im, Sang Chul Kim, Jaemann Kyeong, Hong Soo Park, Joon Hyeop Lee

Hyobin Im et al 2023 The Astronomical Journal 165 .

  • Provider: AAS Journals

Caption: Figure 5.

Best fit PARSEC isochrone line on (a) V vs. (BV) CMD and (b) V vs. (VI) CMD of Czernik 30. The black open circle symbols are the member stars of Czernik 30, the blue open circles indicate the RC stars of Czernik 30, the gray dots are nonmember stars but located inside the radius of Czernik 30 and the red lines are the best fit PARSEC isochrone model.

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