Merger history of central galaxies in Semi-Analytic Models of galaxy formation
Mojtaba Raouf, Habib G. Khosroshahi, Gary A. Mamon, Darren J., Croton, Abdolhosein Hashemizadeh, Ali A. Dariush

TL;DR
This study examines how the dynamical history of galaxy groups influences the evolution of their central galaxies, velocity dispersions, and AGN activity, revealing differences based on formation epoch and group mass.
Contribution
It provides new insights into the dynamical evolution of galaxies in groups with different formation times using semi-analytic models, highlighting the impact of formation epoch on galaxy mergers and velocity dispersion.
Findings
Brightest galaxies in young groups have recent major mergers.
Velocity dispersion increases in dwarf galaxies of young groups.
Radio luminosity of central galaxies correlates with halo assembly history.
Abstract
We investigate the dynamical evolution of galaxies in groups with different formation epochs. Galaxy groups have been selected to be in different dynamical states, namely dynamically old and dynamically young, which reflect their early and late formation times, respectively, based on their halo mass assembly. Brightest galaxies in dynamically young groups have suffered their last major galaxy merger typically Gyr more recently than their counterparts in dynamically old groups. Furthermore, we study the evolution of velocity dispersion in these two classes and compare them with the analytic models of isolated halos. The velocity dispersion of dwarf galaxies in high mass, dynamically young groups increases slowly in time, while the analogous dispersion in dynamically old high-mass groups is constant. In contrast, the velocity dispersion of giant galaxies in low mass groups…
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