The LEGARE Project - I. Chemical evolution model of the Nuclear Stellar Disc in a Bayesian framework

Open Access

Fig. 11

Temporal evolution of inflow gas rate predicted by the models extended for the whole CMZ region, assuming the same total surface mass density of Eq. (7) and multiplied by an area of $π R_{C M Z}^{2}$ $Mathematical equation: $\[\pi R_{C M Z}^{2}\]$$ , where R_CMZ=150 pc. The pink point and associated error bars stand for the value estimated by Hatchfield et al. (2021) using hydrodynamic simulations with AREPO.

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