Radiative transfer in axi-symmetric dust clouds around AGN

Details Radiative transfer in axi-symmetric dust clouds around AGN Radiative transfer in axi-symmetric dust clouds around AGN

May 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992aipc..254..508p&link_type=abstract

In: Testing the AGN paradigm; Proceedings of the 2nd Annual Topical Astrophysics Conference, Univ. of Maryland, College Park, Oc

Astronomy and Astrophysics

Astrophysics

1

Active Galactic Nuclei, Cosmic Dust, Optical Thickness, Radiative Transfer, Thermal Emission, Angular Distribution, Line Of Sight, Spectral Line Width, Symmetry

Scientific paper

We have developed a new radiative transfer code to study the thermally
reradiated emission from an optically and geometrically thick torus of
dusk which partially obscures the central regions of an active galactic
nucleus. We discuss the spectral and angular distributions of the
radiated energy over a range of model parameters and viewing angles.

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