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Fig. 6.

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Distribution of galaxy-integrated CO line ratios obtained for our sample of ULIRGs, with mean and median values reported at the top right of each plot. Left: . Middle: . Right: . The mean CO line ratios measured by Leroy et al. (2022) in local massive main-sequence disk galaxies are shown using vertical dotted lines, with the gray shaded regions representing their 16-84 velocity percentile ranges.

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