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Fig. 3


Ratio between the molecular gas mass, mapped along the major axis with the IRAM 30 m telescope, and extrapolated to the entire disk assuming azimuthal symmetry (MH2,   map,   extra) and the molecular gas mass extrapolated from the central pointing as explained in Sect. 3.5.1 (MH2) as a function of diameter a) and galaxy inclination b).

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