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

Open Access

Fig. 6

Time evolution of the gas density in the central regions of the CHEM_MHD simulations. This is the same as Fig. 5, but zooming-in in the central region. The interior of the CMZ gas ring is empty at t = 147 Myr and then is gradually filled with gas due to MRI-driven accretion (Sect. 7).

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