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Dust Formation in AGN Winds

  • Authors: Arkaprabha Sarangi, Eli Dwek, and Demos Kazanas

2019 The Astrophysical Journal 885 126.

  • Provider: AAS Journals

Caption: Figure 13.

The color map shows the maximum grain sizes at a given region (﹩r,\theta ﹩) where the grains have grown by accretion of free metals in the gas along the flow lines. The black lines in the figure represent the parabolic flow lines with various starting/launch radii on the accretion disk, r0.

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