HyGAL: Characterizing the Galactic ISM with observations of hydrides and other small molecules - II. The absorption line survey with the IRAM 30 m telescope

Open Access

Fig. 7

Same as Fig. 3 but toward G45.07+0.13. The shaded areas indicate the velocity intervals of specific spiral arms (local arm in cyan and Sagittarius-Carina arm in magenta), and the molecular cloud envelope or unidentified foreground clouds in brown.

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