Fitted UBV magnitude for MS stars
收藏B2FIND2026-03-19 收录
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https://b2find.eudat.eu/dataset/76642d21-cbdb-584e-9f8b-e18e9de977ec
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We fit the colour-magnitude diagrams of stars between the zero-age main-sequence and terminal-age main sequence in young clusters and associations. The ages we derive are a...
