EFFECTS OF BARYON DISSIPATION ON THE DARK MATTER VIRIAL SCALING RELATION

We investigate effects of baryon dissipation on the dark matter virial scaling relation between total mass and velocity dispersion and the velocity bias of galaxies in groups and clusters using self-consistent cosmological simulations. We show that the baryon dissipation increases the velocity dispersion of dark matter within the virial radius by approximate to 5%-10%. The effect is mainly driven by the change in density and gravitational potential in inner regions of cluster, and it is larger in lower mass systems where gas cooling and star formation are more efficient. We also show that the galaxy velocity bias depends on how galaxies are selected. Galaxies selected based on their stellar mass exhibit no velocity bias, while galaxies selected based on their total mass show positive bias of approximate to 10%, consistent with previous results based on collisionless dark matter only simulations. We further find that observational estimates of galaxy velocity dispersion are unbiased with respect to the velocity dispersion of dark matter, provided galaxies are selected using their stellar masses and their velocity dispersions are computed with more than 20 most massive galaxies. Velocity dispersions estimated with fewer galaxies, on the other hand, can lead to a significant underestimate of dynamical masses. Results presented in this paper should be useful in interpreting high-redshift groups and clusters as well as cosmological constraints derived from upcoming optical cluster surveys.