An Etymological Dictionary of Astronomy and Astrophysics

A vast, turbulent region encircling the → Milky Way’s nucleus that contains a large fraction of the → Galaxy’s dense → molecular clouds and → star formation regions. Spanning -1 to +1.5 degrees of → Sgr A*, the CMZ is about 400 pc × 100 pc in size and contains at least 10⁷→ solar masses of → giant molecular clouds,
approximately 10% of the Galaxy’s molecular gas. The gas in the CMZ is at higher temperature than typical giant molecular clouds
and has high velocity dispersion reflecting the → turbulent nature of the gas in the area.

Despite these extensive molecular reserves, the → star formation rate within the CMZ is actually lower than expected based on the analysis of nearby → star-forming regions in the quiescent → Galactic disk. A common assumption is that this is a result of the extreme conditions within the CMZ, where the density, pressure, temperature, → velocity dispersion and → radiation field are all significantly greater than elsewhere in the Milky Way (Clark et al. 2018, The Messenger 173, 22 and references therein).

See also: → central; → molecular; → zone.