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Using data from the GAIA-ESO spectroscopic survey, we describe the determination of spectroscopic and stellar parameters of circa 400 low-mass members of the Lagoon Nebula. Based on this analysis, we discuss the luminosity/age spread in the H-R diagram, lithium evolution and place in our findings in context of recent theoretical and observational works. We also compare our results with time-series and near-mid infrared data.
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