3D radiative transfer modelling of the dusty tori around active galactic nuclei as a clumpy two-phase medium
Marko Stalevski(Ghent University), Luka Č. Popović(Chinese Academy of Sciences), M. Baes(HOGENT University of Applied Sciences and Arts), J. Fritz, Theodoros Nakos(Ghent University)
Cited by 406
Related Papers
The Herschel ATLAS
|Publications of the Astronomical Society of the Pacific|2010|603
Tracing the cosmic growth of supermassive black holes to z ∼ 3 with Herschel★
|Monthly Notices of the Royal Astronomical Society|2014|193
Smooth and clumpy dust distributions in AGN: a direct comparison of two commonly explored infrared emission models
|Monthly Notices of the Royal Astronomical Society|2012|192
The Galaxy Activity, Torus, and Outflow Survey (GATOS)
|Astronomy and Astrophysics|2021|144
The flux ratio of the [O III] 5007, 4959 lines in AGN: comparison with theoretical calculations
|Monthly Notices of the Royal Astronomical Society|2006|132