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Fig. 12

image

Images of high-mass irregular LSB galaxies (log M> 9.5, top panel) and high-mass regular LSB galaxies (log M> 9.5, bottom panel). From top left to bottom right in the top panel, the 3rd, 5th, 6th, 8th, 9th, 10th, 12th, and 15th show that either multiple components, double nuclei, or tidal features are all proof of merging.

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