Imagen de Portada

The XMAGNET exascale MHD simulations of SMBH feedback in galaxy groups and clusters: Overview and preliminary cluster results

Fuente: arXiv

Guardado en:

Detalles Bibliográficos
Autores principales:	Grete, Philipp, O'Shea, Brian W., Glines, Forrest W., Prasad, Deovrat, Wibking, Benjamin D., Fournier, Martin, Brüggen, Marcus, Voit, Mark
Formato:	Preprint
Publicado:	2025
Materias:	Astrophysics of Galaxies High Energy Astrophysical Phenomena
Acceso en línea:	Acceder al recurso
Etiquetas:	Agregar Etiqueta Sin Etiquetas, Sea el primero en etiquetar este registro!

Ejemplares similares

XMAGNET : Kinetic, Thermal and Magnetic AGN Feedback in Massive Galaxies at Halo Masses $\sim 10^{13.5}$ M$_\odot$
por: Prasad, Deovrat, et al.
Publicado: (2025)

The properties of magnetised cold filaments in a cool-core galaxy cluster
por: Fournier, Martin, et al.
Publicado: (2024)

XMAGNET: Velocity structure functions of active galactic nucleus-driven turbulence in the multiphase intracluster medium
por: Fournier, M., et al.
Publicado: (2025)

XMAGNET -- Stir before serving: a Lagrangian perspective on mixing-driven condensation in the intracluster medium
por: Fournier, M., et al.
Publicado: (2026)

The Case for Hot-Mode Accretion in Abell 2029
por: Prasad, Deovrat, et al.
Publicado: (2023)

Precipitation possible: turbulence-driven thermal instability with constrained entropy profiles
por: Wibking, Benjamin D., et al.
Publicado: (2024)

Precipitation plausible: magnetized thermal instability in the intracluster medium
por: Wibking, Benjamin D., et al.
Publicado: (2025)

Dynamical friction and measurements of the splashback radius in galaxy clusters
por: O'Shea, Talia M., et al.
Publicado: (2024)

Seeking Self-Regulating Simulations of Idealized Milky Way-Like Galaxies
por: Kopenhafer, Claire, et al.
Publicado: (2022)

Semi-Supervised Rotation Measure Deconvolution and its application to MeerKAT observations of galaxy clusters
por: Gustafsson, Victor, et al.
Publicado: (2024)

Simulations of galaxy cluster mergers with velocity-dependent, rare and frequent self-interactions
por: Sabarish, V. M., et al.
Publicado: (2023)

Stellar-wind feedback and magnetic fields around young compact star clusters: 3D MHD simulations
por: Härer, Lucia, et al.
Publicado: (2025)

The Density Distribution of Compressively-Forced Supersonic Turbulence Depends on the Driving Correlation Time
por: Grete, Philipp, et al.
Publicado: (2025)

An Improved Fit to the Density Distribution in Supersonic Isothermal Turbulence
por: Scannapieco, Evan, et al.
Publicado: (2025)

Deciphering baryonic feedback with galaxy clusters
por: To, Chun-Hao, et al.
Publicado: (2024)

Magnetohydrodynamic Precipitation
por: Voit, G. M., et al.
Publicado: (2026)

A New Superbubble Finding Algorithm: Description and Testing
por: Wallin, Brock, et al.
Publicado: (2024)

Shells and bubbles around compact clusters of massive stars: 3D MHD simulations
por: Badmaev, D. V., et al.
Publicado: (2026)

The Three Hundred Project: The relationship between the shock and splashback radii of simulated galaxy clusters
por: Zhang, M., et al.
Publicado: (2024)

Cosmological simulations of the generation of cluster-scale radio emission from turbulent re-acceleration
por: Beduzzi, Luca, et al.
Publicado: (2024)

Galaxy Assembly and Evolution in the P-Millennium simulation: galaxy clustering
por: Fontanot, Fabio, et al.
Publicado: (2024)

Hydrostatic mass bias for galaxy groups and clusters in the FLAMINGO simulations
por: Braspenning, Joey, et al.
Publicado: (2024)

The alignment between brightest cluster galaxies and host clusters
por: Yuan, Z. S., et al.
Publicado: (2022)

The impact of feedback on the evolution of gas density profiles from galaxies to clusters: a universal fitting formula from the Simba suite of simulations
por: Sorini, Daniele, et al.
Publicado: (2024)

Radio relics in massive galaxy cluster mergers in the TNG-Cluster simulation
por: Lee, W., et al.
Publicado: (2023)

Cosmic dance in the Shapley Concentration Core II. The uGMRT-MeerKAT view of filaments in the brightest cluster galaxies and tailed radio galaxies in the A3528 cluster complex
por: Di Gennaro, G., et al.
Publicado: (2024)

Simulating images of radio galaxies with diffusion models
por: Martínez, Tobias Vičánek, et al.
Publicado: (2024)

The life of central radio galaxies in clusters: AGN-ICM studies of eRASS1 clusters in the ASKAP fields
por: Veronica, Angie, et al.
Publicado: (2025)

ViCTORIA project: The LOFAR-MeerKAT view of AGN in Virgo cluster early-type galaxies
por: Spasic, A., et al.
Publicado: (2024)

Bridging observations and simulations: a machine learning approach to galaxy clusters
por: Gatuzz, Efrain
Publicado: (2025)

Simulating AGN feedback in galaxy clusters with pre-existing turbulence
por: Li, Jia-Lun, et al.
Publicado: (2025)

Merging cold front and AGN feedback in the peculiar galaxy cluster Abell 2626
por: Kadam, Sonali K., et al.
Publicado: (2019)

The history and mass content of cluster galaxies in the EAGLE simulation
por: Sifón, Cristóbal, et al.
Publicado: (2023)

Tidally induced bar-like galaxies in simulated clusters
por: Lokas, Ewa L.
Publicado: (2025)

Deep Learning generated observations of galaxy clusters from dark-matter-only simulations
por: Caro, Andrés, et al.
Publicado: (2024)

How to count clustered galaxies
por: Wang, Yunting, et al.
Publicado: (2026)

AGNs in massive galaxy clusters: Role of galaxy merging, infalling groups, cluster mass, and dynamical state
por: Koulouridis, E., et al.
Publicado: (2024)

The full iron budget in simulated galaxy clusters: The chemistry between gas and stars
por: Biffi, Veronica, et al.
Publicado: (2025)

Memoirs of mass accretion: probing the edges of intracluster light in simulated galaxy clusters
por: Dacunha, Tara, et al.
Publicado: (2025)

Lyman-$α$ feedback prevails at Cosmic Dawn: Implications for the first galaxies, stars, and star clusters
por: Nebrin, Olof, et al.
Publicado: (2024)