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Fig. 11.
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Histogram of ΔCCO and ΔCmol for pure SF, composite, and Seyfert galaxies. ΔCCO (ΔCmol) is the difference between the measured CCO (Cmol) and, at the measured strength, the value of the best-fit CCO-(2 + log sdisk) (Cmol-(2 + log sdisk)) relation constructed using pure SF galaxies as shown in Fig. 10.
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