A survey of molecular clouds in the Galactic center’s outflow

Open Access

Fig. 1

Sample of high-velocity clouds studied in this work. The grayscale map represents the MW disk (Lockman & McClure-Griffiths 2016) and the blue color-scale map the outflowing Hi high-velocity clouds (Di Teodoro et al. 2018). Red circles mark the clouds followed- up in the ¹²CO(2→1) and ¹²CO(4→3) lines with APEX and analyzed in this work, numbered as in Table 1. Dotted gray circles denote clouds not detected in CO emission.

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