Exploring Magnetic Tower Simulation Results Using Astrobear
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- 3D model of mass loading and knot formation in AGN jets by stellar wind. You see an AGB star (orange, horizontally moving ...
- Shocked clump @ 1536 --
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- Gravoturbulent Fragmentation in 2D --
- Jet over clumps,
In-Depth Information on Magnetic Tower Simulation Results Using Astrobear
Rotating (left) vs non-rotating (right) Density VS Beta, Adiabatic-- By Martín Huarte-Espinosa. Clumpy jet Shocked clump @ 192 in 3D --
Shock Triggered Star Formation: Initial Cloud: stable Bonnor-Ebert sphere. Mach = 1.5, non-rotational.
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