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Fig. 7.

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The SAM after the disk phase jfinal for different stellar magnetic field values and stellar masses of 0.1 M (panel a), 0.3 M (panel b), and 0.5 M (panel c). The colored circles, crosses, and squares represent initial rotation periods of 1, 3, and 10 days, respectively, and the solid, dash-dotted, and dashed lines show the respective fits. Mean and standard deviation values for the SAM taken from Somers et al. (2017) are represented by gray solid and dashed lines, respectively.

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