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Fig. 16


Relationship between the CAS parameters determined in the Hα+[NII] narrow band filter and the total stellar mass (left), the stellar mass surface density (centre left), the metallicity (centre right), and the specific star formation rate (right) for HI-normal (HI - def ≤ 0.4; filled dots) and HI-deficient (HI - def > 0.4; empty circles) galaxies.

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