De re metallica: the cosmic chemical evolution of galaxies

R Maiolino, F Mannucci - The Astronomy and Astrophysics Review, 2019 - Springer
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 …

The GLASS-JWST early release science program. I. Survey design and release plans

T Treu, G Roberts-Borsani, M Bradac… - The Astrophysical …, 2022 - iopscience.iop.org
Abstract The GLASS-JWST Early Release Science (hereafter GLASS-JWST-ERS) Program
will obtain and make publicly available the deepest extragalactic data of the ERS campaign …

FIRE-2 simulations: physics versus numerics in galaxy formation

PF Hopkins, A Wetzel, D Kereš… - Monthly Notices of …, 2018 - academic.oup.com
ABSTRACT The Feedback In Realistic Environments (FIRE) project explores feedback in
cosmological galaxy formation simulations. Previous FIRE simulations used an identical …

Reconstructing the last major merger of the Milky Way with the H3 survey

RP Naidu, C Conroy, A Bonaca, D Zaritsky… - The Astrophysical …, 2021 - iopscience.iop.org
Several lines of evidence suggest that the Milky Way underwent a major merger at z∼ 2 with
the Gaia-Sausage-Enceladus (GSE) galaxy. Here we use H3 Survey data to argue that GSE …

What causes the formation of discs and end of bursty star formation?

PF Hopkins, AB Gurvich, X Shen… - Monthly Notices of …, 2023 - academic.oup.com
As they grow, galaxies can transition from irregular/spheroidal with 'bursty'star formation
histories (SFHs), to discy with smooth SFHs. But even in simulations, the direct physical …

[PDF][PDF] Black holes on FIRE: stellar feedback limits early feeding of galactic nuclei

D Anglés-Alcázar, CA Faucher-Giguère… - Monthly Notices of …, 2017 - academic.oup.com
We introduce massive black holes (BHs) in the Feedback In Realistic Environments (FIRE)
project and perform high-resolution cosmological hydrodynamic simulations of quasar-mass …

Be it therefore resolved: cosmological simulations of dwarf galaxies with 30 solar mass resolution

C Wheeler, PF Hopkins, AB Pace… - Monthly Notices of …, 2019 - academic.oup.com
We study a suite of extremely high-resolution cosmological Feedback in Realistic
Environments simulations of dwarf galaxies (), run to z= 0 with resolution, sufficient (for the …

The SINS/zC-SINF Survey of z∼ 2 Galaxy Kinematics: SINFONI Adaptive Optics–assisted Data and Kiloparsec-scale Emission-line Properties∗

NMF Schreiber, A Renzini, C Mancini… - The Astrophysical …, 2018 - iopscience.iop.org
We present the" SINS/zC-SINF AO survey" of 35 star-forming galaxies, the largest sample
with deep adaptive optics (AO)–assisted near-infrared integral field spectroscopy at z∼ 2 …

But what about...: cosmic rays, magnetic fields, conduction, and viscosity in galaxy formation

PF Hopkins, TK Chan… - Monthly Notices of …, 2020 - academic.oup.com
We present and study a large suite of high-resolution cosmological zoom-in simulations,
using the FIRE-2 treatment of mechanical and radiative feedback from massive stars …

Cosmic ray feedback in the FIRE simulations: Constraining cosmic ray propagation with GeV γ-ray emission

TK Chan, D Kereš, PF Hopkins… - Monthly Notices of …, 2019 - academic.oup.com
We present the implementation and the first results of cosmic ray (CR) feedback in the
Feedback In Realistic Environments (FIRE) simulations. We investigate CR feedback in non …