The diversification and dissipation of protoplanetary disks

Open Access

Fig. 4

Threshold accretion rate below which a wind cannot effectively shield the disk from PE-driving X-ray radiation, vs. stellar mass. Curves are calculations for different rotation periods and ages of 1–10 Myr, and points are values of ${\dot{M}}_{acc}$ $\dot{M}_{\rm acc}$ from Manara et al. (2023).

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