All Figures

	Figure 1: 12.2 GHz spectra of the newly detected methanol sources. For this presentation they have been smoothed with the Hanning function.
Open with DEXTER


In the text

	Figure 1: continued.
Open with DEXTER


In the text

	Figure 2: Comparison of fluxes in the detected 12.2 and 6.7 GHz emissions. Gray bins at the right side show all sources with fluxes exceeding the level of 200 Jy km s-1.
Open with DEXTER


In the text

	Figure 3: The velocity dispersion of spectral features for 12.2 and 6.7 GHz. Dashed line marks equality region of the plot. Only a few 12.2 GHz sources have wider line's groups then the same lines at 6.7 GHz.
Open with DEXTER


In the text

Figure 4: A comparison of spectra of three sources. Top panels of each box show 6.7 GHz spectra, and the bottom ones contain 12.2 GHz spectra at similar radial velocity. The top box presents the 6.7 GHz emission and observed huge absorption at 12.2 GHz in 18217-1252. Middle and bottom pairs of spectra show 6.7 GHz absorptions at the radial velocity of 12.2 GHz emission features for 19186-1440 and 21381+5000.

Open with DEXTER


In the text

	Figure 5: The comparison of 6.7 and 12.3 GHz line morphology for sources with spectral features in similar velocity ranges. Upper panels of double boxes contain 6.7 GHz lines, and bottom ones are with 12.2 GHz features. Some of the 12.2 GHz spectra are incomplete within the box boundaries because of nonflat baselines and noises.
Open with DEXTER


In the text

	Figure 5: continued.
Open with DEXTER


In the text

	Figure 5: continued.
Open with DEXTER


In the text

	Figure 5: continued.
Open with DEXTER


In the text