Supernova-driven galactic winds fall into three regimes set by the ratio of supernova scale height to gas scale height, which controls how much mass, metals, and energy escape.
R., Wisnioski E., Acharyya A., Federrath C., Forbes J
6 Pith papers cite this work, alongside 45 external citations. Polarity classification is still indexing.
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COLIBRE simulations find the galaxy gas-phase MZR already in place at z≈10 with little evolution until z≈5, then shallowens at low z, with high-mass turnover set by AGN feedback and low-mass end by core-collapse supernovae.
Te-Te relations from five auroral lines in four low-metallicity starbursts, including diffuse extraplanar gas, are consistent with spiral H II region relations, with one flagged exception.
For future AO-assisted spectrographs, the Blue line suite best recovers metallicities of star-forming galaxies and the LRed suite best recovers AGN-host metallicities, with H-beta SNR of about 10 needed for noise below 0.1 dex.
After placing local and distant galaxy abundances on a common scale, the authors find Milky Way high-alpha disc patterns at z~2-3, evidence for alpha-bimodality in M31, and place the MW and GSE on the z~3 mass-metallicity relation.
DESI spectra yield radial metallicity gradients in 2291 low-z star-forming galaxies that decline steeply in massive systems, flatten at large radii across all masses, and correlate with size and outer stellar age.
citing papers explorer
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QUOKKA-based understanding of outflows (QED) -- III. Outflow loading and phase structure as a function of galactic environment
Supernova-driven galactic winds fall into three regimes set by the ratio of supernova scale height to gas scale height, which controls how much mass, metals, and energy escape.
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The evolution of the galaxy gas-phase mass-metallicity relation from $z=15$ to $z=0$ in the COLIBRE cosmological simulations
COLIBRE simulations find the galaxy gas-phase MZR already in place at z≈10 with little evolution until z≈5, then shallowens at low z, with high-mass turnover set by AGN feedback and low-mass end by core-collapse supernovae.
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Electron temperature relations in low metallicity, diffuse, and extraplanar gas of starburst galaxies
Te-Te relations from five auroral lines in four low-metallicity starbursts, including diffuse extraplanar gas, are consistent with spiral H II region relations, with one flagged exception.
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Optimal strategies for measuring gas-phase metallicities in intermediate-redshift non-AGN and AGN-host galaxies using future instrumentation
For future AO-assisted spectrographs, the Blue line suite best recovers metallicities of star-forming galaxies and the LRed suite best recovers AGN-host metallicities, with H-beta SNR of about 10 needed for noise below 0.1 dex.
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ChemZz I: Comparing Oxygen and Iron Abundance Patterns in the Milky Way, the Local Group and Cosmic Noon
After placing local and distant galaxy abundances on a common scale, the authors find Milky Way high-alpha disc patterns at z~2-3, evidence for alpha-bimodality in M31, and place the MW and GSE on the z~3 mass-metallicity relation.
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DESI as sparse Integral Field Spectrograph I: Spatially resolved chemical enrichment in star-forming galaxies at $z\leq0.1$
DESI spectra yield radial metallicity gradients in 2291 low-z star-forming galaxies that decline steeply in massive systems, flatten at large radii across all masses, and correlate with size and outer stellar age.