Modeling disks and magnetic outflows around a forming massive star - I. Investigating the two-layer structure of the accretion disk

Open Access

Fig. 5

Magnetic Reynolds number, computed with the fiducial simulation on grid ×8. For t = 10 kyr, the radius of the disk is around 80 au, while for t = 22.75 kyr, the exterior radius is ≈700 au and the interior radius is ≈20 au.

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