Simulations of relativistic jet formation in radio sources
Radio galaxies and quasars produce collimated, relativistic flows with. Lorentz factors of at least 15. It is generally believed that such flow Velocities indicate that jet acceleration and collimation occurs in the relativistic environment of a supermassive black hole. Recently, several groups arou...
Main Author: | Meier, D |
---|---|
Format: | Conference item |
Published: |
2002
|
Similar Items
-
A Simulation Study of Low-power Relativistic Jets: Flow Dynamics and Radio Morphology of FR-I Jets
by: Ayan Bhattacharjee, et al.
Published: (2024-01-01) -
Decelerating relativistic radio jets in B2 0755+379
by: Bondi, M, et al.
Published: (2002) -
Multiwavelength Observations of Relativistic Jets from General Relativistic Magnetohydrodynamic Simulations
by: Richard Anantua, et al.
Published: (2018-03-01) -
A relativistic jet in the radio-quiet quasar PG1407+263
by: Blundell, K, et al.
Published: (2003) -
Relativistic Jet Motion in the Radio-quiet LINER Galaxy KISSR 872
by: Preeti Kharb, et al.
Published: (2024-01-01)