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Fig. 7


Normalized cumulative distributions in period associated with the full sample of NGC 2264 members (left panel), the population of CTTS (middle panel), and the population of WTTS (right panel) analyzed in this study. Two prominent jumps of similar extent (0.16 and 0.17) appear in the cumulative distribution for the full sample at P = 1 d and P = 3 d, respectively. In the case of the CTTS, only one prominent jump of 0.21 at P = 3 d is seen. In the case of the WTTS, two prominent discontinuities can again be observed, one steeper at P = 1 d (0.21) and one smaller at P = 3 d (0.15).

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