Fig. 16
Aflux ratio versus spiral strength (Qs) for 40 CIG galaxies overlapping between the H i sample and the CIG galaxies in Durbala et al. (2009). The fit to the data points (slope and intercept are –0.34 and 1.16, Pearson’s correlation coefficient ρ = −0.45) is shown as a (red) solid line. The six outliers have been ignored in this fit.
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