Studies of Low Luminosity Active Galactic Nuclei with Monte Carlo and Magnetohydrodynamic Simulations
Results from several studies are presented which detail explorations of the physical and spectral properties of low luminosity active galactic nuclei. An initial Sagittarius A* general relativistic magnetohydrodynamic simulation and Monte Carlo radiation transport model suggests accretion rate chan...
Main Author: | Hilburn, Guy |
---|---|
Other Authors: | Liang, Edison P. |
Format: | Others |
Language: | English |
Published: |
2012
|
Subjects: | |
Online Access: | http://hdl.handle.net/1911/64694 |
Similar Items
-
Possible Wormhole Candidates in Active Galactic Nuclei
by: Mikhail Piotrovich, et al.
Published: (2020-08-01) -
On the Heating of AGN Magnetospheres
by: Zaza Osmanov, et al.
Published: (2021-03-01) -
Measuring the physical properties of active galactic nuclei
by: Raimundo, Sandra Isabel de Jesus
Published: (2011) -
Magnetohydrodynamic Turbulence and Angular Momentum Transport in Accretion Disks
by: Pessah, Martin Elias
Published: (2007) -
Investigating the nature of dual active galactic nuclei in Stripe 82
by: Gross, Arran Connor
Published: (2019)