De re metallica: the cosmic chemical evolution of galaxies
The evolution of the content of heavy elements in galaxies, the relative chemical
abundances, their spatial distribution, and how these scale with various galactic properties …
abundances, their spatial distribution, and how these scale with various galactic properties …
A comprehensive measurement of the local value of the Hubble constant with 1 km s− 1 Mpc− 1 uncertainty from the Hubble Space Telescope and the SH0ES team
We report observations from the Hubble Space Telescope (HST) of Cepheid variables in the
host galaxies of 42 Type Ia supernovae (SNe Ia) used to calibrate the Hubble constant (H 0) …
host galaxies of 42 Type Ia supernovae (SNe Ia) used to calibrate the Hubble constant (H 0) …
The mass–metallicity and the fundamental metallicity relation revisited on a fully Te-based abundance scale for galaxies
The relationships between stellar mass, gas-phase metallicity and star-formation rate (ie the
mass–metallicity, MZR, and the fundamental metallicity relation, FMR) in the local Universe …
mass–metallicity, MZR, and the fundamental metallicity relation, FMR) in the local Universe …
The MOSDEF survey: direct-method metallicities and ISM conditions at z ∼ 1.5–3.5
We present detections of [O iii] λ4363 and direct-method metallicities for star-forming
galaxies at z= 1.7–3.6. We combine new measurements from the MOSFIRE Deep Evolution …
galaxies at z= 1.7–3.6. We combine new measurements from the MOSFIRE Deep Evolution …
New fully empirical calibrations of strong-line metallicity indicators in star forming galaxies
We derive new empirical calibrations for strong-line diagnostics of gas phase metallicity in
local star forming galaxies by uniformly applying the Te method over the full metallicity range …
local star forming galaxies by uniformly applying the Te method over the full metallicity range …
Past, Present, and Future of the Scaling Relations of Galaxies and Active Galactic Nuclei
M D'Onofrio, P Marziani, C Chiosi - Frontiers in Astronomy and Space …, 2021 - frontiersin.org
We review the properties of the established Scaling Relations (SRs) of galaxies and active
galactic nuclei (AGN), focusing on their origin and expected evolution back in time, providing …
galactic nuclei (AGN), focusing on their origin and expected evolution back in time, providing …
CHAOS IV: Gas-phase Abundance Trends from the First Four CHAOS Galaxies
The chemical abundances of spiral galaxies, as probed by H ii regions across their disks,
are key to understanding the evolution of galaxies over a wide range of environments. We …
are key to understanding the evolution of galaxies over a wide range of environments. We …
Nebular spectroscopy: a guide on H ii regions and planetary nebulae
M Peimbert, A Peimbert… - Publications of the …, 2017 - iopscience.iop.org
We present a tutorial on the determination of the physical conditions and chemical
abundances in gaseous nebulae. We also include a brief review of recent results on the …
abundances in gaseous nebulae. We also include a brief review of recent results on the …
The mass–metallicity relation revisited with CALIFA
We present an updated version of the mass–metallicity (MZ) relation using integral field
spectroscopy data obtained from 734 galaxies observed by the CALIFA survey. These …
spectroscopy data obtained from 734 galaxies observed by the CALIFA survey. These …
Metallicity, ionization parameter, and pressure variations of H ii regions in the TYPHOON spiral galaxies: NGC 1566, NGC 2835, NGC 3521, NGC 5068, NGC 5236 …
K Grasha, QH Chen, AJ Battisti… - The Astrophysical …, 2022 - iopscience.iop.org
We present a spatially resolved H ii region study of the gas-phase metallicity, ionization
parameter, and interstellar medium (ISM) pressure maps of six local star-forming and face …
parameter, and interstellar medium (ISM) pressure maps of six local star-forming and face …