Effective equation of state of a radiatively cooling gas: Self-similar solution of spherical collapse

Fuente: arXiv

Salvato in:

Dettagli Bibliografici
Autore principale:	Lee, Yueh-Ning
Natura:	Preprint
Pubblicazione:	2024
Soggetti:	Astrophysics of Galaxies
Accesso online:	Acceder al recurso
Tags:	Aggiungi Tag Nessun Tag, puoi essere il primo ad aggiungerne!!

Documenti analoghi

Protostellar Disk Formation Regimes: Angular Momentum Conservation versus Magnetic Braking
di: Yen, Hsi-Wei, et al.
Pubblicazione: (2024)

On the minimum number of radiation field parameters to specify gas cooling and heating functions
di: Robinson, David, et al.
Pubblicazione: (2024)

Modeling the cool gas clumps in the circumgalactic medium
di: Yang, Hang, et al.
Pubblicazione: (2025)

Black holes regulate cool gas accretion in massive galaxies
di: Wang, Tao, et al.
Pubblicazione: (2023)

Amplification and saturation of turbulent magnetic field in collapsing primordial gas clouds
di: Higashi, Sho, et al.
Pubblicazione: (2024)

21cm signal from Dark Ages collapsing halos with detailed molecular cooling treatment
di: Plombat, Hugo, et al.
Pubblicazione: (2024)

The complex effect of gas cooling and turbulence on AGN-driven outflow properties
di: Zubovas, K., et al.
Pubblicazione: (2024)

The abundance and origin of cool gas in galaxy clusters in the TNG-Cluster simulation
di: Staffehl, Milan, et al.
Pubblicazione: (2025)

Molecular gas in cool-core brightest cluster galaxies at $z\simeq0.4$
di: Castignani, G., et al.
Pubblicazione: (2025)

Magnetohydrodynamical modeling of star-disk formation: from isolated spherical collapse towards incorporation of external dynamics
di: Kuffmeier, M.
Pubblicazione: (2024)

The MUSE Ultra Deep Field (MUDF) VIII. The cool gas distribution surrounding galaxies at redshifts z ~ 0.5-2
di: Santo, Edoardo, et al.
Pubblicazione: (2026)

General non-linear fragmentation with discontinuous Galerkin methods
di: Lombart, Maxime, et al.
Pubblicazione: (2024)

The First Estimation of the Ambipolar Diffusivity Coefficient from Multi-Scale Observations of the Class 0/I Protostar, HOPS-370
di: Thieme, Travis J., et al.
Pubblicazione: (2024)

MUSE Analysis of Gas around Galaxies (MAGG) -- VI. The cool and enriched gas environment of z$\gtrsim$3 Ly$α$ emitters
di: Galbiati, Marta, et al.
Pubblicazione: (2024)

Dust evolution during the protostellar collapse: influence on the coupling between the neutral gas and the magnetic field
di: Vallucci-Goy, Valentin, et al.
Pubblicazione: (2024)

Hybrid-chimes: A model for radiative cooling and the abundances of ions and molecules in simulations of galaxy formation
di: Ploeckinger, Sylvia, et al.
Pubblicazione: (2025)

Self-similar decomposition of the hierarchical merger tree of dark matter halos
di: Jiang, Wenkang, et al.
Pubblicazione: (2025)

Quasar radiation transforms the gas in a merging companion galaxy
di: Balashev, Sergei, et al.
Pubblicazione: (2025)

Self-similarity of the magnetic field at different scales: the case of G31.41+0.31
di: Beltrán, M. T., et al.
Pubblicazione: (2024)

The Rotation Dip in the Envelope-Disk Transition of HH 111: Evidence for Magnetic Braking
di: Lin, Jyun-Heng, et al.
Pubblicazione: (2025)

Formation of the Little Red Dots from the Core-collapse of Self-interacting Dark Matter Halos
di: Jiang, Fangzhou, et al.
Pubblicazione: (2025)

The impact of shear on the rotation of Galactic plane molecular clouds
di: Rani, Raffaele, et al.
Pubblicazione: (2024)

Why is the Galactic disk so cool?
di: Hamilton, Chris, et al.
Pubblicazione: (2024)

Population III star formation: multiple gas phases prevent the use of an equation of state at high densities
di: Prole, Lewis R., et al.
Pubblicazione: (2023)

On the properties and implications of collapse-driven MHD turbulence
di: Vázquez-Semadeni, Enrique, et al.
Pubblicazione: (2024)

Bonnor-Ebert sphere collapse in filamentary structures
di: Heigl, Stefan, et al.
Pubblicazione: (2026)

Self-similar cluster structures in massive star-forming regions: Isolated evolution from clumps to embedded clusters
di: Zhou, J. W., et al.
Pubblicazione: (2024)

Ambipolar diffusion and the mass-to-flux ratio in a turbulent collapsing cloud
di: Tritsis, Aris
Pubblicazione: (2025)

Probing cold gas with Mg II and Ly$α$ radiative transfer
di: Chang, Seok-Jun, et al.
Pubblicazione: (2024)

The evolution of molecular clouds: turbulence-regulated global radial collapse
di: Luo, An-Xu, et al.
Pubblicazione: (2024)

Little Red Dots as Direct-collapse Black Hole Nurseries
di: Cenci, Elia, et al.
Pubblicazione: (2025)

Tracing the evolution of the cool gas in CGM and IGM environments through Mg II absorption from redshift z=0.75 to z=1.65 using DESI-Y1 data
di: Wu, X., et al.
Pubblicazione: (2024)

Deep Learning solutions to singular ordinary differential equations: from special functions to spherical accretion
di: Cayuso, R., et al.
Pubblicazione: (2024)

Gravothermal collapse and the diversity of galactic rotation curves
di: Roberts, M. Grant, et al.
Pubblicazione: (2024)

An nl-model with a full radiative transfer treatment for level populations of hydrogen atoms in a spherically symmetric H II region
di: Zhu, F. -Y., et al.
Pubblicazione: (2025)

Quiescent fractions in high-redshift galaxy groups reflect their hot-or-cold state of gas accretion
di: Elias, Guillaume, et al.
Pubblicazione: (2026)

The heart of galaxy clusters: demographics and physical properties of cool-core and non-cool-core halos in the TNG-Cluster simulation
di: Lehle, Katrin, et al.
Pubblicazione: (2023)

The effects of different cooling and heating function models on a simulated analog of NGC300
di: Robinson, David, et al.
Pubblicazione: (2024)

When self-similarity meets mass spectrum and anisotropy
di: Pavlík, Václav
Pubblicazione: (2026)

Ultraviolet diversity of Little Red Dots as a probe for direct-collapse black hole ages
di: Cenci, Elia, et al.
Pubblicazione: (2026)