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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 14.

The color map shows the dust-to-gas mass ratio in polar coordinates (r, θ). The white region is the sublimation zone, and the black lines indicate flow lines with various launch radii r0. The mass ratio seems to be larger toward the longer radii, outward of 3 × 1018 cm, where the ratio is ∼10−2.

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