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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 11.

Dust-to-gas number density ratio along three different inclinations, θ = 30°, 75°, and 85°, presented as a function of the radial distance from the central source, with reference to the gas number density shown in Figure 3 (bottom left) and the dust number density in Figure 10.

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