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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 5.

Normalized amplitude profiles A( r)/Σ 0( r) of unstable modes A 1 and A 2 for model 1 in Table 2. Top: classical KBOs reside at the accumulation point, and we have set . The current semimajor axes of the orbits of Saturn and Neptune are indicated by vertical dotted lines. Bottom: unstable modes are fit to the inner solar system with . The mean semimajor axis of the most populous asteroid belt and the present semimajor axes of the terrestrial planets have been indicated by vertical dotted lines.

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