Simulations of Precessing Jets and the Formation of X-shaped Radio Galaxies
Jet precession is sometimes invoked to explain asymmetries in radio galaxy (RG) jets and “X/S/Z-shaped” RGs, caused by the presence of a binary black hole companion to the source active galactic nucleus or by accretion instabilities. We present a series of simulations of RG jet precession to examine...
Main Authors: | Chris Nolting, Jay Ball, Tri M. Nguyen |
---|---|
Format: | Article |
Language: | English |
Published: |
IOP Publishing
2023-01-01
|
Series: | The Astrophysical Journal |
Subjects: | |
Online Access: | https://doi.org/10.3847/1538-4357/acc652 |
Similar Items
-
The Connection between the Radio Jet and the γ-ray Emission in the Radio Galaxy 3C 120 and the Blazar CTA 102
by: Carolina Casadio, et al.
Published: (2016-09-01) -
Radio Jet Feedback on the Inner Disk of Virgo Spiral Galaxy Messier 58
by: Patrick M. Ogle, et al.
Published: (2024-01-01) -
X-shaped radio galaxies: probing jet evolution, ambient medium dynamics, and their intricate interconnection
by: Gourab Giri, et al.
Published: (2024-03-01) -
Remnant Radio Galaxy Candidates of Small Angular Sizes
by: Veeresh Singh, et al.
Published: (2021-12-01) -
Deciphering the Morphological Origins of X-shaped Radio Galaxies: Numerical Modeling of Backflow versus Jet Reorientation
by: Gourab Giri, et al.
Published: (2023-01-01)