Physics – Fluid Dynamics
Scientist
Physics
Fluid Dynamics
Scientist
Department of Mechanical and Industrial Engineering, Concordia University
A classical flow instability and its connection to gaseous galactic disk hydrodynamics
Mixing Within Patterned Vortex Core
Particle paths of Lagrangian velocity distribution simulating the spiral arms of galaxy M51
Sunspots are in many ways similar to terrestrial vortices
The presence of interstellar turbulence could explain the velocity flattening in galaxies
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