Image de couverture de livre

Why are thermally- and cosmic ray-driven galactic winds fundamentally different?

Fuente: arXiv

Enregistré dans:

Détails bibliographiques
Auteurs principaux:	Thomas, Timon, Pfrommer, Christoph, Pakmor, Rüdiger
Format:	Preprint
Publié:	2024
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

Effective cosmic ray diffusion in multiphase galactic environments
par: Thomas, Timon, et autres
Publié: (2025)

CRexit: how different cosmic ray transport modes affect thermal instability in the circumgalactic medium
par: Weber, Matthias, et autres
Publié: (2025)

The theory of resonant cosmic ray-driven instabilities -- Growth and saturation of single modes
par: Lemmerz, Rouven, et autres
Publié: (2024)

Anisotropic thermal conduction on a moving mesh for cosmological simulations
par: Talbot, Rosie Y., et autres
Publié: (2024)

The magnetised and thermally unstable tails of jellyfish galaxies
par: Sparre, Martin, et autres
Publié: (2023)

SPICE: the connection between cosmic reionisation and stellar feedback in the first galaxies
par: Bhagwat, Aniket, et autres
Publié: (2023)

Steady-State or Not? The Evolution of Cosmic Ray Electron Spectra in Galaxies
par: Werhahn, Maria, et autres
Publié: (2025)

Cosmic Ray-Driven Galactic Winds with Resolved ISM and Ion-Neutral Damping
par: Sike, Brandon, et autres
Publié: (2024)

Unveiling the Impact of Cosmic Rays on the Disc Sizes and Outflows from Dwarf Scales to Galaxy Groups
par: Bieri, Rebekka, et autres
Publié: (2025)

Axionlike dark-matter winds driven by galactic baryon redistribution
par: Nazarenko, A. V.
Publié: (2026)

Simulating Radio Synchrotron Morphology, Spectra, and Polarization of Cosmic Ray Driven Galactic Winds
par: Chiu, H. -H. Sandy, et autres
Publié: (2024)

Robust magnetic field estimates in star-forming galaxies with the equipartition formula in the absence of equipartition
par: Chiu, H. -H. Sandy, et autres
Publié: (2025)

The dynamical impact of cosmic rays in the Rhea magnetohydrodynamics simulations
par: Kjellgren, Karin, et autres
Publié: (2025)

Cascading from the winds to the disk: the universality of supernovae-driven turbulence in different galactic interstellar media
par: Connor, Isabelle, et autres
Publié: (2025)

Simulating cosmic ray electron spectra and radio emission from an AGN jet outburst in a cool-core cluster
par: Jlassi, Léna, et autres
Publié: (2026)

When are galactic winds molecular?
par: Vijayan, Aditi, et autres
Publié: (2024)

Magnetohydrodynamic turbulence and the associated spatial diffusion tensor of cosmic rays in dynamical galactic halos
par: Kleimann, J., et autres
Publié: (2025)

Cloud properties in simulated galactic winds
par: Warren, Orlando, et autres
Publié: (2024)

Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback
par: Sike, Brandon, et autres
Publié: (2025)

Magnetic dynamos in galaxy clusters: the crucial role of galaxy formation physics at high redshifts
par: Tevlin, Larissa, et autres
Publié: (2024)

How supermassive black holes shape central entropies in galaxy clusters
par: Weinberger, Rainer, et autres
Publié: (2026)

Comparing the interstellar and circumgalactic origin of gas in the tails of jellyfish galaxies
par: Sparre, Martin, et autres
Publié: (2024)

The emergence of galactic thin and thick discs across cosmic history
par: Tsukui, Takafumi, et autres
Publié: (2024)

Revisiting radio synchrotron diagnostics in star-forming galaxies
par: Werhahn, Maria, et autres
Publié: (2026)

Magnetic field amplification in cosmological zoom simulations from dwarf galaxies to galaxy groups
par: Pakmor, Ruediger, et autres
Publié: (2023)

Connecting outflows with radio emission in active galactic nuclei at cosmic noon
par: Ilha, Gabriele S., et autres
Publié: (2025)

The major merger-active galactic nucleus connection up to the cosmic noon
par: La Marca, A., et autres
Publié: (2026)

The boundary of cosmic filaments
par: Wang, Wei, et autres
Publié: (2024)

Identifying heating processes in simulations with an entropy-based scheme: A single jet episode in a galaxy cluster
par: Meenakshi, Moun, et autres
Publié: (2026)

Characterizing turbulence in galaxy clusters: defining turbulent energies and assessing multi-scale versus fixed-scale filters
par: Perrone, Lorenzo Maria, et autres
Publié: (2026)

Galactic bars and active galactic nucleus fuelling in the second half of cosmic history
par: La Marca, A., et autres
Publié: (2025)

FEASTS Compared with Simulations: Abnormally Irregular and Extended HI Morphologies at a Column Density of $10^{18}\,\text{cm}^{-2}$ in TNG50 and Auriga
par: Lin, Xuchen, et autres
Publié: (2025)

Quokka-based understanding of outflows (QED) -- II. X-ray metallicity gradients as a signature of galactic wind metal loading
par: Huang, Rongjun, et autres
Publié: (2024)

Survival and synthetic observables of neutral atomic hydrogen in galactic wind simulations
par: Banda-Barragán, Wladimir E., et autres
Publié: (2024)

Hydrodynamic shielding in radiative multicloud outflows within multiphase galactic winds
par: Villares, Andrés S., et autres
Publié: (2024)

Bridging Scales: Coupling the galactic nucleus to the larger cosmic environment
par: Su, Kung-Yi, et autres
Publié: (2024)

Ion densities of cold clouds driven by galactic outflows
par: Yang, Lisiyuan, et autres
Publié: (2025)

QED V: Variations in metal loading of galactic winds with element nucleosynthetic origin
par: Vijayan, Aditi, et autres
Publié: (2026)

An analytical galactic chemical evolution model with gas inflow and a terminal wind
par: Kvasova, Kateryna A., et autres
Publié: (2025)

The extent of intergalactic metal enrichment from galactic winds during the Cosmic Dawn
par: Yamaguchi, Natsuko, et autres
Publié: (2022)