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.
Silvio Ariel Alfaro (Tue,) studied this question.
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