NGC6530 member parameters from Gaia-ESO survey

Name: NGC6530 member parameters from Gaia-ESO survey
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B2FIND2026-03-19 收录

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https://b2find.eudat.eu/dataset/50fecabe-d3a6-5f65-920f-5a049b70d436

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In very young clusters, stellar age distribution is the empirical proof of the duration of star formation (SF) and of the physical mechanisms involved in the process. We derived...