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Article overview
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The cosmic evolution of the stellar mass-velocity dispersion relation of early-type galaxies | Carlo Cannarozzo
; Alessandro Sonnenfeld
; Carlo Nipoti
; | Date: |
15 Oct 2019 | Abstract: | Taking 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 | Services: | Forum | Review | PDF | Favorites |
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