Central Molecular Zone
The Central Molecular Zone is a distinct region of intense molecular gas concentration and heightened star formation activity located in the inner few hundred parsecs of the Milky Way Galaxy, distinguished from other galactic molecular complexes by its extreme physical conditions, including high gas densities, temperatures, and turbulent velocities, within the broader context of galactic nuclei environments.
176
Publications
11.1K
Citations
687
Authors
343
Institutions
Publications per year
2017–2026
99
Variants
Cmz
Parents
176
THE GALACTIC CENTER ENVIRONMENT
M. Morris, Eugene Serabyn · Annual Review of Astronomy and Astrophysics · 1996 · 943 citations
Natural Sciences, Astronomy, Physics +16
J. M. Diederik Kruijssen, J. E. Dale, Steven N. Longmore · Monthly Notices of the Royal Astronomical Society · 2014 · 240 citations · Full text
Natural Sciences, Astronomy, Physics +17
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687
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Center for Astrophysics Harvard & Smithsonian, United States
21 publications · 1.8K citations
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15
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1–5 of 687
343
Heidelberg University
Heidelberg, Germany
31 h-index
76 publications
4.7K citations
Liverpool John Moores University
Liverpool, United Kingdom
27 h-index
50 publications
4.1K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
25 h-index
54 publications
3.1K citations
Max Planck Institute for Radio Astronomy
Bonn, Germany
23 h-index
67 publications
4.6K citations
National Astronomical Observatory of Japan
Mitaka-shi, Japan
23 h-index
49 publications
2.2K citations
Max Planck Institute for Astronomy
Heidelberg, Germany
22 h-index
65 publications
3.4K citations
National Radio Astronomy Observatory
Charlottesville, United States
21 h-index
45 publications
2.9K citations

Atacama Large Millimeter Submillimeter Array
Santiago, Chile
19 h-index
25 publications
1.4K citations
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45 publications · 3.3K citations
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ApJ · 38 publications · 2.2K citations
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30 publications · 1.6K citations
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12 publications · 851 citations
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8 publications · 266 citations
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