Search Results - "Porter, Lori E"
-
1
Spatially resolved gas-phase metallicity in FIRE-2 dwarfs: late-time evolution of metallicity relations in simulations with feedback and mergers
Published in Monthly notices of the Royal Astronomical Society (05-08-2022)“…ABSTRACT We present an analysis of spatially resolved gas-phase metallicity relations in five dwarf galaxies ($\rm \mathit{M}_{halo} \approx 10^{11}\, {\rm…”
Get full text
Journal Article -
2
The loneliest galaxies in the Universe: a GAMA and Galaxy Zoo study on void galaxy morphology
Published in Monthly notices of the Royal Astronomical Society (01-10-2023)“…ABSTRACT The large-scale structure of the Universe is comprised of galaxy filaments, tendrils, and voids. The majority of the Universe’s volume is taken up by…”
Get full text
Journal Article -
3
Any way the wind blows: quantifying superbubbles and their outflows in simulated galaxies across z ≈ 0 − 3
Published in Monthly notices of the Royal Astronomical Society (15-11-2024)“…We present an investigation of clustered stellar feedback in the form of superbubbles identified within eleven galaxies from the FIRE-2 (Feedback in Realistic…”
Get full text
Journal Article -
4
Any Way the Wind Blows: Quantifying Superbubbles and their Outflows in Simulated Galaxies across $z \approx 0-3
Published 05-06-2024“…We present an investigation of clustered stellar feedback in the form of superbubbles identified within eleven galaxies from the FIRE-2 (Feedback in Realistic…”
Get full text
Journal Article -
5
The Loneliest Galaxies in the Universe: A GAMA and GalaxyZoo Study on Void Galaxy Morphology
Published 12-04-2023“…The large-scale structure (LSS) of the Universe is comprised of galaxy filaments, tendrils, and voids. The majority of the Universe's volume is taken up by…”
Get full text
Journal Article -
6
Spatially Resolved Gas-phase Metallicity in FIRE-2 Dwarfs: Late-Time Evolution of Metallicity Relations in Simulations with Feedback and Mergers
Published 13-04-2022“…We present an analysis of spatially resolved gas-phase metallicity relations in five dwarf galaxies ($M_{halo} \approx 10^{11} M_\odot$, $M_\star \approx…”
Get full text
Journal Article