Article
Extended Data Table 1 | Properties of molecular gas clouds outflowing from the Galactic Centre
Shown are the Galactic coordinates (l, b); the height from the Galactic plane (z); the distance from the Galactic Centre (r) from our biconical outflow model^12 ; the peak^12 CO(2 → 1) brightness
temperature (Tb,peak); typical CO line widths (FWHM); the velocity range of the CO line in the LSR; the lower limits to the molecular masses (Mmol), derived from^12 CO(2 → 1) data; and atomic gas
masses (Mat), derived from H i data. Masses include helium.