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Fig. A.2

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Spectra of individual 6.7 GHz maser clouds with Gaussian velocity profiles. Each circle traces the emission level of a single maser spot as presented in Figs. 1 and A.1. The black line represents the fitting of a Gaussian function (or functions) as summarized in Table B.1. The gray line presents the single Gaussian fitting in a case of complex velocity profile of an individual component.

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