Fig3

A plot showing the measured rotational velocity of each galaxy in the sample versus its luminosity. The dashed lines show the scatter around the Tully Fisher relation. Galaxies in the different sample classes tend to reside in different locations on the plot.

A plot showing the measured rotational velocity of each galaxy in the sample versus its luminosity. The dashed lines show the scatter around the Tully Fisher relation. Galaxies in the different sample classes tend to reside in different locations on the plot.

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