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Global Drag-induced Instabilities in Protoplanetary Disks

  • Authors: Mir Abbas Jalali

Jalali 2013 The Astrophysical Journal 772 75.

  • Provider: AAS Journals

Caption: Figure 4.

Variation of the amplitude profile A( R) of modes A 1 and A 2 in models with different mass parameters and drag coefficients. See Table 2 for the specifications of the models. The difference between models 6 and 10 is indistinguishable in the plots. The R-axis is in logarithmic scale.

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