Star Formation in Disk Galaxies

Rosemary F. G. Wyse , Annette M. N. Ferguson , Jay Gallagher , Deidre Hunter, PASA, 15 (1), 118
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As noted in Binney & Tremaine (1987), section 5.3.1, the similarity in instability criteria is due to the fact that the unstable scale-length in the zero-thickness case is much larger than the disk thickness.
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