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20242026
most citedMagnetic field morphology and evolution in the Central Molecular Zone and its effect on gas dynamics

28 citations · 42 across the 20 of their papers we have counts for

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astro-ph.GA2024

3-D CMZ II: Hierarchical Structure Analysis of the Central Molecular Zone

Cara Battersby, Daniel L. Walker, Ashley Barnes +16

The Central Molecular Zone (CMZ) is the way station at the heart of our Milky Way Galaxy, connecting gas flowing in from Galactic scales with the central nucleus. Key open question…

astro-ph.GA2024

3-D CMZ III: Constraining the 3-D structure of the Central Molecular Zone via molecular line emission and absorption

Daniel L. Walker, Cara Battersby, Dani Lipman +15

The Milky Way's Central Molecular Zone (CMZ) is the largest concentration of dense molecular gas in the Galaxy, the structure of which is shaped by the complex interplay between Ga…

astro-ph.GA2024

3-D CMZ I: Central Molecular Zone Overview

Cara Battersby, Daniel L. Walker, Ashley Barnes +16

The Central Molecular Zone (CMZ) is the largest reservoir of dense molecular gas in the Galaxy and is heavily obscured in the optical and near-IR. We present an overview of the far…

astro-ph.GA2024★ 14 cited

3-D CMZ IV: Distinguishing Near vs. Far Distances in the Galactic Center Using Spitzer and Herschel

Dani Lipman, Cara Battersby, Daniel L. Walker +15

A comprehensive 3-D model of the central 300 pc of the Milky Way, the Central Molecular Zone (CMZ) is of fundamental importance in understanding energy cycles in galactic nuclei, s…

astro-ph.GA2024★ 28 cited

Magnetic field morphology and evolution in the Central Molecular Zone and its effect on gas dynamics

R. G. Tress, M. C. Sormani, P. Girichidis +34

The interstellar medium in the Milky Way's Central Molecular Zone (CMZ) is known to be strongly magnetised, but its large-scale morphology and impact on the gas dynamics are not we…