THE PREVALENCE OF GAS OUTFLOWS IN TYPE 2 AGNs. II. 3D BICONICAL OUTFLOW MODELS

ABSTRACT We present 3D models of biconical outflows combined with a thin dust plane for investigating the physical properties of the ionized gas outflows and their effect on the observed gas kinematics in type 2 active galactic nuclei (AGNs). Using a set of input parameters, we construct a number of...

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Veröffentlicht in:	The Astrophysical journal 2016-09, Vol.828 (2), p.97-97
Hauptverfasser:	Bae, Hyun-Jin, Woo, Jong-Hak
Format:	Artikel
Sprache:	eng
Schlagworte:	Active galactic nuclei ASTROPHYSICS, COSMOLOGY AND ASTRONOMY COMPARATIVE EVALUATIONS Computer simulation COMPUTERIZED SIMULATION COSMIC DUST Dispersion DISPERSIONS DISTRIBUTION EMISSION GALAXIES galaxies: active galaxies: kinematics and dynamics GALAXY NUCLEI Inclination Mathematical models methods: analytical MONTE CARLO METHOD Outflow PHYSICAL PROPERTIES Three dimensional models THREE-DIMENSIONAL CALCULATIONS VELOCITY
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