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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 4.

Ratio of the luminosities transmitted through the column of outflowing gas from the accretion disk, compared to the source luminosities, for two inclinations, θ = 30°, 75°. Owing to the larger column densities and high densities along high inclination angles, a larger fraction of the source luminosity is absorbed by the gas.

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