none11si©: 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.The coevolution of galaxies and their metal content serves as an important test for galaxy feedback models. We analyse the distribution and evolution of metals within the IllustrisTNG simulation suite with a focus on the gas-phase mass−metallicity relation (MZR). We find that the IllustrisTNG model broadly reproduces the slope and normalization evolution of the MZR across the redshift range 0 2) evolution fit by d log(Z)/dz ≈ −0.064. Our simulations indicate that the metal retention efficiency of the interstellar medium (ISM) is low: a majority of gas-phase metals (∼85 per cent at z = 0) live outside of the IS...
International audienceWe present a new measurement of the gas-phase mass-metallicity relation (MZR) ...
The fundamental metallicity relation (FMR) is a postulated correlation between galaxy stellar mass, ...
In this paper, we take advantage of the GAlaxy Evolution and Assembly (GAEA) semi-analytic model to...
The coevolution of galaxies and their metal content serves as an important test for galaxy feedback ...
The coevolution of galaxies and their metal content serves as an important test for galaxy feedback ...
The coevolution of galaxies and their metal content serves as an important test for galaxy feedback ...
The coevolution of galaxies and their metal content serves as an important test for galaxy feedback ...
The evolution of the metal content of galaxies and its relations to other global properties [such as...
The evolution of the metal content of galaxies and its relations to other global properties [such as...
We investigate the evolution of galaxy gas-phase metallicity (O/H) over the range z = 0-3.3 using sa...
We present the stellar mass–stellar metallicity relationship (MZR) in the galaxy cluster Cl0024+1654...
none13siThis article has been accepted for publication in MNRAS Letters ©: 2018 The Author(s) Publis...
We use the semi-analytic model (SAM) of galaxy formation and evolution SAG coupled with the MULTIDAR...
The fundamental metallicity relation (FMR) is a postulated correlation between galaxy stellar mass, ...
Galaxy evolution can be understood by measuring characteristic properties of the diffuse, ionized ga...
International audienceWe present a new measurement of the gas-phase mass-metallicity relation (MZR) ...
The fundamental metallicity relation (FMR) is a postulated correlation between galaxy stellar mass, ...
In this paper, we take advantage of the GAlaxy Evolution and Assembly (GAEA) semi-analytic model to...
The coevolution of galaxies and their metal content serves as an important test for galaxy feedback ...
The coevolution of galaxies and their metal content serves as an important test for galaxy feedback ...
The coevolution of galaxies and their metal content serves as an important test for galaxy feedback ...
The coevolution of galaxies and their metal content serves as an important test for galaxy feedback ...
The evolution of the metal content of galaxies and its relations to other global properties [such as...
The evolution of the metal content of galaxies and its relations to other global properties [such as...
We investigate the evolution of galaxy gas-phase metallicity (O/H) over the range z = 0-3.3 using sa...
We present the stellar mass–stellar metallicity relationship (MZR) in the galaxy cluster Cl0024+1654...
none13siThis article has been accepted for publication in MNRAS Letters ©: 2018 The Author(s) Publis...
We use the semi-analytic model (SAM) of galaxy formation and evolution SAG coupled with the MULTIDAR...
The fundamental metallicity relation (FMR) is a postulated correlation between galaxy stellar mass, ...
Galaxy evolution can be understood by measuring characteristic properties of the diffuse, ionized ga...
International audienceWe present a new measurement of the gas-phase mass-metallicity relation (MZR) ...
The fundamental metallicity relation (FMR) is a postulated correlation between galaxy stellar mass, ...
In this paper, we take advantage of the GAlaxy Evolution and Assembly (GAEA) semi-analytic model to...