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

Authors

687

  1. JM
    J. M. Diederik Kruijssen

    Heidelberg University, Germany

    27 publications · 2.5K citations

    25

    h-index

  2. SN
    Steven N. Longmore

    Liverpool John Moores University, United Kingdom

    22 publications · 2.2K citations

    20

    h-index

  3. CB
    Cara Battersby

    Center for Astrophysics Harvard & Smithsonian, United States

    21 publications · 1.8K citations

    18

    h-index

  4. AG
    Adam Ginsburg

    National Radio Astronomy Observatory, United States

    17 publications · 818 citations

    15

    h-index

  5. TP
    T. Pillai

    Max Planck Institute for Radio Astronomy, Germany

    14 publications · 739 citations

    14

    h-index

1–5 of 687

Venues

  1. Monthly Notices of the Royal Astronomical Society

    45 publications · 3.3K citations

    28

    h-index

  2. The Astrophysical Journal

    ApJ · 38 publications · 2.2K citations

    25

    h-index

  3. Astronomy and Astrophysics

    30 publications · 1.6K citations

    23

    h-index

  4. The Astrophysical Journal Letters

    12 publications · 851 citations

    11

    h-index

  5. 8

    h-index

1–5