Fig. 1
Continuum emission maps toward the G 19.61−0.23 high-mass star-forming region. All the contour levels are drawn with ± 7σ·2n, where σ is the rms noise level of the image (Table 1) and n = 0,1,2,... . The wavelength and FWHM of the synthesized beam are indicated in the bottom right corner of each panel. See Table 1 for the values of the synthesized beams.
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