First results from the TNG50 simulation: the evolution of stellar and gaseous discs across cosmic time
We present a new cosmological, magnetohydrodynamical simulation for galaxy formation:
TNG50, the third and final instalment of the IllustrisTNG project. TNG50 evolves 2× 21603 …
TNG50, the third and final instalment of the IllustrisTNG project. TNG50 evolves 2× 21603 …
The JWST Hubble sequence: The rest-frame optical evolution of galaxy structure at 1.5< z< 6.5
We present results on the morphological and structural evolution of a total of 3956 galaxies
observed with JWST at 1.5< z< 6.5 in the JWST CEERS observations that overlap with the …
observed with JWST at 1.5< z< 6.5 in the JWST CEERS observations that overlap with the …
Shark: introducing an open source, free, and flexible semi-analytic model of galaxy formation
We present a new, open source, free, semi-analytic model (SAM) of galaxy formation, Shark,
designed to be highly flexible and modular, allowing easy exploration of different physical …
designed to be highly flexible and modular, allowing easy exploration of different physical …
SDSS-IV MaNGA: stellar angular momentum of about 2300 galaxies: unveiling the bimodality of massive galaxy properties
We measure, a proxy for galaxy specific stellar angular momentum within one effective
radius, and the ellipticity, ε, for about 2300 galaxies of all morphological types observed with …
radius, and the ellipticity, ε, for about 2300 galaxies of all morphological types observed with …
Galactic angular momentum in the IllustrisTNG simulation–I. Connection to morphology, halo spin, and black hole mass
We use the TNG100 simulation of the IllustrisTNG project to investigate the stellar specific
angular momenta (j*) of∼ 12 000 central galaxies at z= 0 in a full cosmological context, with …
angular momenta (j*) of∼ 12 000 central galaxies at z= 0 in a full cosmological context, with …
Gas accretion and galactic fountain flows in the Auriga cosmological simulations: angular momentum and metal redistribution
RJJ Grand, F van de Voort, J Zjupa… - Monthly Notices of …, 2019 - academic.oup.com
Using a set of 15 high-resolution magnetohydrodynamic cosmological simulations of Milky
Way formation, we investigate the origin of the baryonic material found in stars at redshift …
Way formation, we investigate the origin of the baryonic material found in stars at redshift …
Deep Extragalactic VIsible Legacy Survey (DEVILS): motivation, design, and target catalogue
LJM Davies, ASG Robotham, SP Driver… - Monthly Notices of …, 2018 - academic.oup.com
ABSTRACT The Deep Extragalactic VIsible Legacy Survey (DEVILS) is a large
spectroscopic campaign at the Anglo-Australian Telescope (AAT) aimed at bridging the near …
spectroscopic campaign at the Anglo-Australian Telescope (AAT) aimed at bridging the near …
The Cosmic Ballet II: spin alignment of galaxies and haloes with large-scale filaments in the EAGLE simulation
We investigate the alignment of galaxies and haloes relative to cosmic web filaments using
the EAGLE hydrodynamical simulation. We identify filaments by applying the nexus+ method …
the EAGLE hydrodynamical simulation. We identify filaments by applying the nexus+ method …
Interacting galaxies on FIRE-2: the connection between enhanced star formation and interstellar gas content
We present a comprehensive suite of high-resolution (parsec-scale), idealized (non-
cosmological) galaxy merger simulations (24 runs, stellar mass ratio∼ 2.5: 1) to investigate …
cosmological) galaxy merger simulations (24 runs, stellar mass ratio∼ 2.5: 1) to investigate …
A fast-rotator post-starburst galaxy quenched by supermassive black-hole feedback at z = 3
The most massive galaxies in the Universe stopped forming stars due to the time-integrated
feedback from central supermassive black holes (SMBHs). However, the exact quenching …
feedback from central supermassive black holes (SMBHs). However, the exact quenching …