Why are there barred spiral galaxies?

Astronomers who construct models of galaxies on supercomputers seem to think that these galaxies arise from an instability that develops in the stellar distribution in the nuclear regions of these galaxies. This gravitational instability causes the orbits of the stars to get locked into a coherent spatial 'structure' with a bar-like shape. It seems that the strength of the bar-like instability has something to do with the mass of the nuclear region such that galaxies with lots of stars in their nuclei are somehow immune from this instability, while galaxies with small nuclei are prone to developing it.
Copyright 1997 Dr. Sten Odenwald
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