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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 16.

Mass absorption coefficient of astronomical silicates, derived from Weingartner & Draine (2001), shown for three different grain radii, a = 0.01, 0.1. and 1 μm, which is the range in which a majority of the grains are present.

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