Image de couverture de livre

The breakBRD Breakdown: Using IllustrisTNG to Track the Quenching of an Observationally-Motivated Sample of Centrally Star-Forming Galaxies

Fuente: arXiv

Enregistré dans:

Détails bibliographiques
Auteurs principaux:	Kopenhafer, Claire, Starkenburg, Tjitske K., Tonnesen, Stephanie, Tuttle, Sarah
Format:	Preprint
Publié:	2020
Sujets:	Astrophysics of Galaxies
Accès en ligne:	Acceder al recurso
Tags:	Ajouter un tag Pas de tags, Soyez le premier à ajouter un tag!

Documents similaires

BreakBRD Galaxies: Evolutionary Clues Through an Analysis of Gas Content
par: Stark, David V., et autres
Publié: (2024)

The History of Galaxy Mergers in IllustrisTNG
par: Koncz, Bendeguz, et autres
Publié: (2025)

Extreme Metallicity Dwarf Galaxies in IllustrisTNG
par: Carleton, Timothy, et autres
Publié: (2024)

Identification of Compact Groups of Galaxies in IllustrisTNG300
par: Yoo, Seungwu, et autres
Publié: (2026)

Galaxy Populations in the IllustrisTNG Caustic Skeleton
par: Hertzsch, Benjamin, et autres
Publié: (2026)

IllustrisTNG in the HSC-SSP: No Shortage of Thin Disk Galaxies in TNG50
par: Xu, Dewang, et autres
Publié: (2024)

Galaxy evolution in groups: Transition galaxies in the IllustrisTNG simulations
par: Levis, Selene, et autres
Publié: (2025)

Enhanced Star Formation and Black Hole Accretion Rates in Galaxy Mergers in IllustrisTNG50
par: Schechter, Aimee L., et autres
Publié: (2025)

Calibrating Galaxy Infall Times in Groups and Clusters with IllustrisTNG Simulations
par: Masson, Florine, et autres
Publié: (2026)

High-redshift Merger-induced Bar-like Galaxies in IllustrisTNG
par: Lokas, Ewa L.
Publié: (2025)

IllustrisTNG Insights: Factors Affecting the Presence of Bars in Disk Galaxies
par: Lu, Shuai, et autres
Publié: (2024)

The Velocity Dispersion Function for Quiescent Galaxies in Massive Clusters from IllustrisTNG
par: Sohn, Jubee, et autres
Publié: (2024)

Environmental effects on Low Surface Brightness Galaxies in the IllustrisTNG simulation
par: Pérez-Montaño, Luis Enrique, et autres
Publié: (2024)

Discrepancies Between JWST Observations and Simulations of Quenched Massive Galaxies at $z > 3$: A Comparative Study With IllustrisTNG and ASTRID
par: Weller, Emma Jane, et autres
Publié: (2024)

Mass and Metal Flows in Isolated IllustrisTNG Halos
par: Morgan, Jacob P., et autres
Publié: (2025)

The formation and evolution of Supermassive disks in IllustrisTNG
par: Pallero, Diego, et autres
Publié: (2025)

Revisiting the bimodality of galactic habitability in IllustrisTNG
par: Mitrašinović, Ana, et autres
Publié: (2025)

Constructing a Galaxy Cluster Catalog in IllustrisTNG-300 using the Mulguisin Algorithm
par: Shin, Lael, et autres
Publié: (2024)

Kinematic morphology of low-mass galaxies in IllustrisTNG
par: Zeng, Guangquan, et autres
Publié: (2024)

The Magellanic Clouds are very rare in the IllustrisTNG simulations
par: Haslbauer, Moritz, et autres
Publié: (2024)

Stellar Metallicity of Galaxies: New Insight on the Formation and Evolution of Low Surface Brightness Galaxies in the IllustrisTNG Simulation
par: Tang, Lin
Publié: (2024)

Quenching pathways in the green valley at low redshift: confronting SDSS AGN hosts with IllustrisTNG and EAGLE
par: Gawade, Gaurav
Publié: (2025)

Describing the Nonuniversal Galaxy Merger Timescales in IllustrisTNG: Effects of Host Halo Mass, Baryons, and Sample Selection
par: Xu, Kun, et autres
Publié: (2025)

The Outskirt Stellar Mass of Low-Redshift Massive Galaxies is an Excellent Halo Mass Proxy in Illustris/IllustrisTNG Simulations
par: Xu, Shuo, et autres
Publié: (2024)

Reconciling the Fundamental Plane of Early-Type Galaxies with hydrodynamical simulations: The case of IllustrisTNG100-1
par: Ferreira, Pedro de Araujo, et autres
Publié: (2026)

Physical Processes Behind the Co-Evolution of Halos, Galaxies and Supermassive Black Holes in the IllustrisTNG Simulation
par: Li, Hao, et autres
Publié: (2024)

The oldest tidally induced bar-like galaxy in the IllustrisTNG cluster
par: Lokas, Ewa L.
Publié: (2025)

Disparate Effects of Circumgalactic Medium Angular Momentum in IllustrisTNG and SIMBA
par: Liu, Kexin, et autres
Publié: (2024)

The Cosmic Baryon Cycle in IllustrisTNG: flows of mass, energy, and metals
par: Oren, Yossi, et autres
Publié: (2025)

Impact of cosmic web on the properties of galaxies in IllustrisTNG simulations
par: Yu, Guangyao, et autres
Publié: (2025)

Polarization-shape alignment of IllustrisTNG star-forming galaxies
par: Zhou, Rui, et autres
Publié: (2025)

Galaxy assembly bias in cosmological hydrodynamical simulations: a comparison between SIMBA and IllustrisTNG
par: Yang, Hong-Gang, et autres
Publié: (2025)

Beyond the Merger-Quasar-Quench Paradigm I: Mergers are neither necessary nor sufficient to quench central galaxies in IllustrisTNG
par: Casimiro, Camilo A., et autres
Publié: (2026)

Puzzling Ultra-Diffuse Galaxy Evolution (PUDGE). I. The existence of a Nube-like galaxy in IllustrisTNG
par: Pavlov, Nataša, et autres
Publié: (2025)

Interplay of Stellar and Gas-Phase Metallicities: Unveiling Insights for Stellar Feedback Modeling with Illustris, IllustrisTNG, and EAGLE
par: Garcia, Alex M., et autres
Publié: (2024)

IllustrisTNG + Cosmic Rays with a Simple Transport Model: From Dwarfs to L$^\star$ Galaxies
par: Ramesh, Rahul, et autres
Publié: (2024)

The splashback radius and the radial velocity profile of galaxy clusters in IllustrisTNG
par: Pizzardo, Michele, et autres
Publié: (2023)

A deep learning model for the density profiles of subhaloes in IllustrisTNG
par: Lucie-Smith, Luisa, et autres
Publié: (2024)

Dynamics of the response of dark matter halo to galaxy evolution in IllustrisTNG
par: Velmani, Premvijay, et autres
Publié: (2024)

Entropy Evolution Towards DARKexp of IllustrisTNG Dark Matter Halos
par: Francis, Ashley, et autres
Publié: (2025)