Inherent and Local Magnetic Field Structures in Jets from Active Galactic Nuclei
In theoretical models for the electromagnetic launching of astrophysical jets, a helical magnetic (<b>B</b>)-field component is generated through the winding up of an initial longitudinal field component by the rotation of the cental black hole and accretion disk. This helical field comp...
| Main Author: | |
|---|---|
| Format: | Article |
| Language: | English |
| Published: |
MDPI AG
2021-08-01
|
| Series: | Galaxies |
| Subjects: | |
| Online Access: | https://www.mdpi.com/2075-4434/9/3/58 |