111 citations · 234 across the 4 of their papers we have counts for
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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…
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…
Simulations of the Milky Way's central molecular zone -- II. Star formation
Mattia C. Sormani, Robin G. Tress, Simon C. O. Glover +5
The Milky Way's central molecular zone (CMZ) has emerged in recent years as a unique laboratory for the study of star formation. Here we use the simulations presented in Tress et a…
Simulations of the Milky Way's central molecular zone -- I. Gas dynamics
Robin G. Tress, Mattia C. Sormani, Simon C. O. Glover +5
We use hydrodynamical simulations to study the Milky Way's central molecular zone (CMZ). The simulations include a non-equilibrium chemical network, the gas self-gravity, star form…