Investigating the IGM and CGM
The intergalactic medium and circumgalactic medium play crucial roles in the formation and evolution of galaxies. One primary research goal is to understand how Mg II absorbers observed in the spectra of background quasars are connected to galaxies.
By analyzing mock quasar absorption spectra generated from cosmological simulations such as IllustrisTNG and SIMBA, this work asks whether absorbers originate from outflowing material expelled by star-forming galaxies or from large rotating disks accreting material onto galaxies.
