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20 April 2024
 
  » arxiv » 1910.6987

 Article overview


The cosmic evolution of the stellar mass-velocity dispersion relation of early-type galaxies
Carlo Cannarozzo ; Alessandro Sonnenfeld ; Carlo Nipoti ;
Date 15 Oct 2019
AbstractTaking advantage of a Bayesian hierarchical inference formalism, we study the evolution of the observed correlation between central stellar velocity dispersion $sigma_0$ and stellar mass $M_*$ of massive ($M_*gtrsim 10^{10.5},mathrm{M_odot}$) early-type galaxies (ETGs) out to redshift $zapprox 2.5$. Collecting ETGs from state-of-the-art literature samples, we consider both a fiducial ($0lesssim zlesssim 1.2$) and an extended ($0lesssim zlesssim 2.5$) samples. Based on the fiducial sample, we find that at $zlesssim 1.2$ the $M_*-sigma_0$ relation is well represented by $sigma_0propto M_*^{eta}(1+z)^{zeta}$, with $etasimeq 0.23$ (at given $z$, $sigma_0$ increases with $M_*$ as a power law with slope similar to the classical Faber-Jackson relation) and $zetasimeq 0.26$ (at given $M_*$, $sigma_0$ decreases for decreasing $z$, for instance by $simeq 20\%$ from $z=1$ to $z=0$). The analysis of the extended sample suggests that over the wider redshift range $0lesssim zlesssim 2.5$ the slope $eta$ could be slightly steeper at higher $z$ ($etasimeq 0.2+0.2log(1+z)$ describes the data as well as constant $etasimeq 0.23$) and that the redshift-dependence of the normalisation could be stronger ($zetasimeq 0.42$). The intrinsic scatter in $sigma_0$ at given $M_*$ is $simeq 0.07$ dex for the fiducial sample at $zlesssim 1.2$, but is found to increase with redshift in the extended sample, being $simeq 0.11$ dex at $z=2$. Our results suggest that, on average, the velocity dispersion of individual massive ($M_*gtrsim 5 imes 10^{11}M_odot$) ETGs decreases with time while they evolve from $zapprox 1$ to $zapprox 0$.
Source arXiv, 1910.6987
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