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Fig. 1


Properties of NGC 2264 members considered in this study (open and filled circles) are compared to those of the full sample of NGC 2264 members available from CSI 2264 (grey dots). Filled circles identify the periodic sources emerging from the analysis in Sect. 3. Mass tracks shown on the diagram and isochrones at 1 Myr (dash-dotted line) and 5 Myr (dotted line) are from Siess et al.’s (2000) models.

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