The most massive stars in very young star clusters with a limited mass: Evidence favours significant self-regulation in the star formation processes

Open Access

Fig. 7.

Standard deviation of M_ecl (blue triangles) and m_max (red squares) for the groups of ten nearest points in the m_max − M_ecl relation. The orange and the blue curves in the upper panel are the synthetic relations assuming optimal sampling of stars. The lower panel shows the difference between the model and the observations.

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