Fig. 9.
Distributions of the sample galaxies as a function of (left) slope α, marking the change in measured J = 1−0 CO flux as a function of increasing observing beam size, (center) the fraction f22 of the extrapolated total galaxy CO flux detected in a 22″ beam, and (right) the extrapolated galaxy CO size as a fraction of the optical size (D25) (see text).
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