24 лютого 2021

Dynamical model of an obscuring clumpy torus in AGNs: I. Velocity and velocity dispersion maps for interpretation of ALMA observations

 Dynamical model of an obscuring clumpy torus in AGNs: I. Velocity and velocity dispersion maps for interpretation of ALMA observations

EY Bannikova, AV Sergeyev, NA Akerman, PP Berczik… - Monthly Notices of the Royal …, 2021
We have developed the dynamical model of a clumpy torus in an active galactic
nucleus (AGN) and compared to recent ALMA observations. We present N-body
simulations of a torus in the field of a supermassive black hole (SMBH), made of up
to N= 105 gravitationally interacting clouds. As initial conditions, we choose random
distributions of the orbital elements of the clouds with a cut-off in the inclination to
mimic the presence of wind cones produced at the early AGN stage. When the torus …
Цитує: ‪CLOUD DISTRIBUTION IN OBSCURING TORI OF ACTIVE …‬  Редагувати



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