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Fig. 4


Simulated evolution of a normal distribution of rotation periods (upper left) emulating that of a 5 Myr-old cluster (see text) at subsequent ages of 13 Myr (upper middle), 25 Myr (upper right), 55 Myr (center left), 130 Myr (center middle), 250 Myr (center right), 550 Myr (lower left), 1.25 Gyr (lower middle), and 2.5 Gyr (lower right).

This figure is made of several images, please see below:

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