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Fig. 8

image

Ratio V/σ as a function of galaxy stellar mass (left panel), maximum rotational velocity (middle panel), and size (right panel). The horizontal dashed lines set the limit between rotation-dominated (blue points above the line) and dispersion-dominated (red points below the line) galaxies. No clear correlation is seen but dispersion-dominated galaxies are mostly massive (>109M), slowly rotating (50 km s-1), and compact.

This figure is made of several images, please see below:

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