1 code implementation • 17 Jun 2016 • Gabriela Calistro Rivera, Elisabeta Lusso, Joseph F. Hennawi, David W. Hogg
The model consists of four physical emission components: an accretion disk, a torus of AGN heated dust, stellar populations, and cold dust in star forming regions.
Astrophysics of Galaxies Instrumentation and Methods for Astrophysics
