:: Library Catalog

Imagen de Portada

Guardado en:

Detalles Bibliográficos
Autores principales:	Whitworth, D. J., Srinivasan, S., Pudritz, R. E., Mac Low, M. -M., Eadie, G., Palau, A., Soler, J. D., Smith, R. J., Pattle, K., Robinson, H., Pillsworth, R., Wadsley, J., Brucy, N., Lebreuilly, U., Hennebelle, P., Girichidis, P., Gent, F. A., Marin, J., Valido, L. Sánchez, Camacho, V., Klessen, R. S., Vázquez-Semadeni, E.
Formato:	Preprint
Publicado:	2024
Materias:	Astrophysics of Galaxies
Acceso en línea:	https://arxiv.org/abs/2407.18293
Etiquetas:	Agregar Etiqueta Sin Etiquetas, Sea el primero en etiquetar este registro!

Ejemplares similares

On the relation between magnetic field strength and gas density in the interstellar medium. II. Density uncertainties and diffuse gas constraints
por: Whitworth, David, et al.
Publicado: (2026)

Filamentary Hierarchies and Superbubbles: Galactic Multiscale MHD Simulations of GMC to Star Cluster Formation
por: Zhao, Bo, et al.
Publicado: (2024)

Necessary conditions for the formation of filaments and star clusters in the cold neutral medium
por: Pillsworth, Rachel, et al.
Publicado: (2024)

What is the contribution of gravitational infall on the mass assembly of star-forming clouds? A case study in a numerical simulation of the interstellar medium
por: Brucy, Noé, et al.
Publicado: (2025)

Cloud properties across spatial scales in simulations of the interstellar medium
por: Colman, Tine, et al.
Publicado: (2024)

Magnetic clumping of charged dust in the dense interstellar medium
por: Vallucci-Goy, V., et al.
Publicado: (2025)

The fragmentation properties of massive star-forming regions in 30Dor-10 at 2000 au resolution
por: Traficante, A., et al.
Publicado: (2026)

Kinetic tomography of the Galactic plane within 1.25 kiloparsecs from the Sun. The interstellar flows revealed by HI and CO line emission and 3D dust
por: Soler, J. D., et al.
Publicado: (2024)

Revealing the Connection Between the Filamentary Hierarchy and Star Cluster Formation in a Simulated NGC 628 Galaxy
por: Koletic, Tamara, et al.
Publicado: (2025)

How is cold, star-forming gas in galaxies affected by magnetic fields?
por: Bogue, Kamran R. J., et al.
Publicado: (2025)

From theory to observation: understanding filamentary flows in high-mass star-forming clusters
por: Wells, M. R. A., et al.
Publicado: (2025)

The accretion luminosity of Class I protostars
por: Testi, L., et al.
Publicado: (2025)

Star Formation and Magnetic Field Amplification due to Galactic Spirals
por: Robinson, Hector, et al.
Publicado: (2025)

Filamentary Hierarchies and Superbubbles II: Impact of superbubbles and galactic dynamics on filament formation and fragmentation
por: Pillsworth, Rachel, et al.
Publicado: (2026)

The signature of large scale turbulence driving on the structure of the interstellar medium
por: Colman, Tine, et al.
Publicado: (2022)

Filamentary accretion flows in high-mass star-forming clouds
por: Schneider, J. -E., et al.
Publicado: (2025)

Evading the dust fragmentation barrier with the streaming instability in protoplanetary disks
por: Vallucci-Goy, V., et al.
Publicado: (2025)

The diffuse gamma-ray sky of a Milky Way analogue: Local diversity and global constraints
por: Kjellgren, Karin, et al.
Publicado: (2026)

Inefficient star formation in high Mach number environments II. Numerical simulations and comparison with analytical models
por: Brucy, Noé, et al.
Publicado: (2024)

Filamentary Hierarchies and Superbubbles I: Characterizing filament properties across a simulated spiral galaxy
por: Pillsworth, Rachel, et al.
Publicado: (2025)

Does supernova feedback regulate the star formation rate in dwarf galaxies?
por: Whitworth, D., et al.
Publicado: (2026)

Planet formation in chemically diverse and evolving discs -- I. Composition of planetary building blocks
por: Pacetti, E., et al.
Publicado: (2025)

Planetesimal formation via the streaming instability in simulations of infall dominated young disks
por: Hühn, L. -A., et al.
Publicado: (2025)

Inefficient star formation in high Mach number environments I. The turbulent support analytical model
por: Hennebelle, Patrick, et al.
Publicado: (2024)

Anisotropy in the carbon monoxide (CO) line emission across the Milky Way's disk
por: Soler, J. D., et al.
Publicado: (2025)

A new multifluid method for dusty astrophysical flows. Application to turbulent protostellar collapses
por: Verrier, Gabriel, et al.
Publicado: (2025)

The role of turbulence in setting the phase of the ISM and implications for the star formation rate
por: Colman, Tine, et al.
Publicado: (2025)

Signatures of magnetic braking in Class 0 protostars ? Exploring the gas kinematics in magnetized models of low-mass star formation
por: Añez-Lopez, N., et al.
Publicado: (2024)

Magnetic field morphology and evolution in the Central Molecular Zone and its effect on gas dynamics
por: Tress, R. G., et al.
Publicado: (2024)

Synthetic populations of protoplanetary disks. Impact of magnetic fields and radiative transfer
por: Lebreuilly, U., et al.
Publicado: (2023)

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

Introducing the Rhea simulations of Milky-Way-like galaxies I: Effect of gravitational potential on morphology and star formation
por: Göller, Junia, et al.
Publicado: (2025)

Rhea-RT: Dynamical impact of Central Molecular Zone conditions on ISM properties and stellar feedback coupling
por: Tress, R. G., et al.
Publicado: (2025)

The fragmentation of molecular clouds in starburst environments
por: Cusack, Matt T., et al.
Publicado: (2025)

The spectrum of magnetized turbulence in the interstellar medium
por: Beattie, James R., et al.
Publicado: (2025)

Do stars still form in molecular gas within CO-dark dwarf galaxies?
por: Whitworth, David J., et al.
Publicado: (2024)

Modeling Local Bubble analogs II: Synthetic Faraday rotation maps
por: Maconi, Efrem, et al.
Publicado: (2025)

Rotational equilibrium of C$_2$ in diffuse interstellar clouds
por: Bourlot, J. Le, et al.
Publicado: (2025)

Microbial Metabolism and Nutrient Cycling in the Mississippi and Atchafalaya River Plumes
por: Pakulski, J., Benner, R., Whitledge, T., Amon, R., Eadie, B., Cifuentes, L., Ammerman, J., Stockwell, D
Publicado: (1993)

Testing kinematic distances under a realistic Galactic potential
por: Hunter, Glen H., et al.
Publicado: (2024)