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Fig. 18


Final parametrization: Intrinsic dispersion (see Sect. 4.6.1) as a function of galactocentric radius (this may be compared with Fig. 13). From top to bottom we show as in Fig. 15 c-C3 H2 (DSP), CH3C2H (DSP-2) and, overlapping, c-C3H2 (DSP-3) andH 42α (DSP-4; see Table 1).

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