Multiparametric analysis reveals stellar population characteristics of NGC 6025, indicating it is a moderately young cluster.
This work presents a multiparametric analysis of the open cluster NGC 6025 (Caldwell 95) using Gaia data. Member stars were selected based on parallax and proper motion constraints. A color–magnitude diagram was constructed to study the stellar population, revealing a well-defined main sequence with spectral types ranging from A to G, consistent with a moderately young cluster.
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Silvio Ariel Alfaro (2026) studied this question.
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