Living on the edge of the Milky Way's central molecular zone - G1.3 is the more likely candidate for gas accretion into the CMZ

Open Access

Fig. B.1

CH₃CN 5_K–4_K and 6_K–5_K spectra at positions P1 to P3 (left to right) in G1.3 (top) and G1.6 (bottom), respectively. The blue curve shows the 1D Gaussian fit. Rest frequencies of all K transitions for each fitted velocity component ci with i = (1, 2) are indicated with vertical lines at the bottom.

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