Spectra and maps of 6.7 GHz methanol masers detected using the EVN. The names are the Galactic coordinates of the brightest spots listed in Table 2. The colors of circles relate to the LSR velocities as shown in the spectra. The map origins are the locations of the brightest spots (Table 2). The gray lines show the Torun 32 m dish spectra. If needed, the separate scale of the flux density is presented on the left (EVN) and right (Torun) sides. The thin bars under the spectra show the LSR velocity ranges of spots displayed. The plots for the first four targets are presented in Fig. 1.

continued. For clarity, in G43.171+00.004, G43.167−0.004, and G43.149+0.013, we listed the LSR velocities in km s^-1 (or LSR velocity range) of a given maser (or maser groups).

continued. In G45.493+00.126 we listed the LSR velocities in km s^-1 (or LSR velocity range) of a given maser (or maser groups).

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.

continued.

continued.

Fit to the spectral energy distribution for the remaining targets.

continued.