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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 2.

Isocontours of the collisional term S 0/( f 0ξ) in the space of orbital elements. Horizontal dashed line corresponds to the mean eccentricity of particle orbits in the initial model. Mass parameters have been set to μ = 0.04 and μ p = 1/8. Particles migrate linear in time toward the accumulation point ( a 0, e 0) ≈ (0.63, 0.128) shown by a cross. Contour lines mark the levels 0.0 to 4 × 10 −4 with steps of 10 −4. Note the logarithmic scale of the a-axis.

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