Image Details

Choose export citation format:

Dust Formation in AGN Winds

  • Authors: Arkaprabha Sarangi, Eli Dwek, and Demos Kazanas

2019 The Astrophysical Journal 885 126.

  • Provider: AAS Journals

Caption: Figure 2.

Luminosity of the central source Lν(θ) is presented for an inclination of θ = 75°, defined in Equation (2). The shape of the spectra is determined by αox = −1.5. For all the inclination angles, the shape of the spectra remains unchanged, whereas the total luminosities vary with f(θ). The material around the AGN is solely heated by the radiation from the central source.

Other Images in This Article

Show More

Copyright and Terms & Conditions

Additional terms of reuse