Simulations on Head-Tail Radio Galaxies Using Magnetic Tower Model
Conference
·
OSTI ID:1212621
- Shenghai Astronomical Observatory
- Los Alamos National Laboratory
The presentation is a series of slides showing diagrams, equations, and various photographs. In summary, a detailed comparison was carried out between hydrodynamic jet and MHD jet models (the magnetic tower jet, more precisely), in an effort to understand the underlying physics of observed radio galaxies, and also its possible indications for jet feedback. It was found that the results of magnetic tower model usually lie in a reasonable regime, and in several aspects, the magnetic tower jet seems more preferred than pure hydrodynamic jet models.
- Research Organization:
- Los Alamos National Laboratory (LANL), Los Alamos, NM (United States)
- Sponsoring Organization:
- USDOE Laboratory Directed Research and Development (LDRD) Program
- DOE Contract Number:
- AC52-06NA25396
- OSTI ID:
- 1212621
- Report Number(s):
- LA-UR-15-26539
- Resource Relation:
- Conference: 5th East-Asia School and Workshop on Laboratory, Space, Astrophysical Plasmas ; 2015-08-17 - 2015-08-22 ; POSTECH, Korea, South
- Country of Publication:
- United States
- Language:
- English
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