Unveiling the galactic baryon cycle process by an empirical model

TL;DR

This paper introduces an empirical model that links galaxy baryon cycle processes with observational and simulation data, revealing how gas recycling and accretion vary with halo mass during galaxy evolution.

Contribution

It presents a novel empirical framework combining star formation, gas content, and metallicity data to constrain baryon cycle processes across different galaxy halo masses.

Findings

Recycled gas fraction increases with halo mass, from 25% to 75%.

Mass loading factors align with FIRE-2 simulation results.

Approximately 70% of baryons are accreted into halos, with 80% of outflowing gas escaping to the IGM.

Abstract

We propose an empirical model to describe and constrain the baryon cycle process during galaxy evolution. This model utilizes the evolution of star formation rate, derived from the stellar mass-halo mass relations (SHMRs) across different redshifts, and the cold gas content, derived from the NeutralUniverseMachine model, to constrain gas accretion and recycle of gas outflow in the model galaxy. Additionally, through detailed modeling of each cycle process, particularly the recycling process, and utilizing the gas-phase mass-metallicity relation (MZR) at $z=0$ as a constraint, our model establishes a relation between the recycle fraction and halo mass. It is found that the fraction of gas recycled from the outflow is a function of halo mass, with a value of $25\%$ in galaxies with halo mass $\sim10^{10.4}M_{\rm \odot}$, increasing to $75\%$ in halos with mass $\sim 10^{12}M_{\rm \odot}$. We also find that the mass loading factor from the FIRE-2 simulation matches well with the constraints from both observational data and our model. Furthermore, using the gas content and metallicity of the circumgalactic medium (CGM) obtained from hydrodynamical simulations as constraints, our model predicts that on average $70\%$ of universal baryon accretion is accreted to the halo and $80\%$ of the non-recycled gas in the outflow has escaped from the galaxy, entering the intergalactic medium (IGM). However, we note that future observational data are needed to finally constrain the mass and metal exchange between the CGM and the IGM.