Image de couverture de livre

Jellyfish galaxies with the IllustrisTNG simulations -- When, where, and for how long does ram pressure stripping of cold gas occur?

Fuente: arXiv

Enregistré dans:

Détails bibliographiques
Auteurs principaux:	Rohr, Eric, Pillepich, Annalisa, Nelson, Dylan, Zinger, Elad, Joshi, Gandhali, Ayromlou, Mohommadreza
Format:	Preprint
Publié:	2023
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

Jellyfish galaxies with the IllustrisTNG simulations -- Supermassive black hole activity in dense environments with ram-pressure stripped satellites
par: Kurinchi-Vendhan, Shalini, et autres
Publié: (2025)

The hot circumgalactic media of massive cluster satellites in the TNG-Cluster simulation: existence and detectability
par: Rohr, Eric, et autres
Publié: (2023)

The cooler past of the intracluster medium in TNG-Cluster
par: Rohr, Eric, et autres
Publié: (2024)

The abundance and origin of cool gas in galaxy clusters in the TNG-Cluster simulation
par: Staffehl, Milan, et autres
Publié: (2025)

Numerical effects on the stripping of dark matter and stars in IllustrisTNG galaxy groups and clusters
par: Lovell, Mark R., et autres
Publié: (2025)

ERGO-ML: Comparing IllustrisTNG and HSC galaxy images via contrastive learning
par: Eisert, Lukas, et autres
Publié: (2023)

The diverse physical origins of stars in the dynamically hot bulge: CALIFA vs. IllustrisTNG
par: Zhang, Le, et autres
Publié: (2025)

Mass Proxy Quality of Massive Halo Properties in the IllustrisTNG and FLAMINGO Simulations: I. Hot Gas
par: Aljamal, Eddie, et autres
Publié: (2025)

Introducing the TNG-Cluster Simulation: overview and physical properties of the gaseous intracluster medium
par: Nelson, Dylan, et autres
Publié: (2023)

The heart of galaxy clusters: demographics and physical properties of cool-core and non-cool-core halos in the TNG-Cluster simulation
par: Lehle, Katrin, et autres
Publié: (2023)

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

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

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

An Atlas of Gas Motions in the TNG-Cluster Simulation: from Cluster Cores to the Outskirts
par: Ayromlou, Mohammadreza, et autres
Publié: (2023)

Cosmic gas accretion from filaments onto galaxy clusters using the IllustrisTNG simulation
par: Pasté, Jade, et autres
Publié: (2026)

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

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

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

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

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

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

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

Study of barred galaxies in IllustrisTNG100: the case of low surface brightness galaxies
par: Chim-Ramirez, Karol, et autres
Publié: (2025)

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

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

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

X-ray-inferred kinematics of the core ICM in Perseus-like clusters: Insights from the TNG-Cluster simulation
par: Truong, Nhut, et autres
Publié: (2023)

Interacting galaxies in the IllustrisTNG simulations -- VI: Reconstructed orbits, close encounters and mergers
par: Patton, David R., et autres
Publié: (2024)

What Drives Cluster Cool-Core Transformations? A Population Level Analysis of TNG-Cluster
par: Lehle, Katrin, et autres
Publié: (2025)

IllustrisTNG in the HSC-SSP: No Shortage of Thin Disk Galaxies in TNG50
par: Xu, Dewang, 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)

Introducing cosmosTNG: simulating galaxy formation with constrained realizations of the COSMOS field
par: Byrohl, Chris, et autres
Publié: (2024)

Tracing correlations between galaxy properties across the Cosmic Web: An IllustrisTNG-based study
par: Nandi, Anindita, et autres
Publié: (2025)

The catalogue of virtual early-type galaxies from IllustrisTNG: validation and real observation consistency
par: Ferreira, Pedro de Araujo, et autres
Publié: (2025)

Interacting galaxies in the IllustrisTNG simulations - IX: Mini mergers trigger AGN in cosmological simulations
par: Byrne-Mamahit, Shoshannah, et autres
Publié: (2025)

Unifying the dynamical classification of early-type galaxies: kinematic deficits in IllustrisTNG versus observations
par: Zhong, Wenyu, et autres
Publié: (2026)

Introducing the AIDA-TNG project: galaxy formation in alternative dark matter models
par: Despali, Giulia, et autres
Publié: (2025)

Quantifying the unwinding due to ram pressure stripping in simulated galaxies
par: Machado, Rubens E. G., et autres
Publié: (2025)