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. 2021 Jan 1;7(1):eaba5967. doi: 10.1126/sciadv.aba5967

Fig. 2. Regions in the disk where various hydrodynamic instabilities may operate.

Fig. 2

Shown are the estimated locations where each of three hydrodynamic instabilities—the VSI (blue), COS (white), and ZVI (red)—is expected to dominate based on cooling time calculations for a specific disk model and under the assumption that magnetic fields are not present. Adopted from (15) with permission.