Figure 14 from Dust Formation in AGN Winds

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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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