Galaxy Cyclonics and Relativistic Jets

A fraction of oscillating fluid densities in the bubble film experiments (1995-2012) have evolved into rotating rings or cyclonic structures void of any center (torus-like). The phenomenon occurs mainly in regular and superelliptical pentagonal frames.

Recent observations from the Event Horizon Telescope teams (2019) have detailed the accretion disk activity of a black hole. Black hole and cyclonic ring images are identical suggesting the BH is simply another oscillating density galaxy phase or active cyclonic ring, which impacts the formation and radiation of relativistic jets.

Blurred cyclonic ring image with 2019 EHT Black Hole picture

Image of Centaurus A radio galaxy with jets and lobes extending out of the central region.

Credits: NASA/CXC/CfA

A rotating cyclonic ring extracting energy from the oscillating galactic nucleus emits relativistic jets.

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