Imagen de Portada

Scales of Stability and Turbulence in the Molecular ISM

Fuente: arXiv

Guardado en:

Detalles Bibliográficos
Autor principal:	Keto, Eric
Formato:	Preprint
Publicado:	2024
Materias:	Astrophysics of Galaxies
Acceso en línea:	Acceder al recurso
Etiquetas:	Agregar Etiqueta Sin Etiquetas, Sea el primero en etiquetar este registro!

Ejemplares similares

Apparent Stability in Self-Gravitating Turbulence and the Evolution of Molecular Clouds
por: Keto, Eric
Publicado: (2026)

Scales of Stability and Turbulence in the Molecular ISM
por: Eric Keto
Publicado: (2024)

Analytic Modeling of CO Surface-Density Profiles in the M31 Molecular Clouds
por: Keto, Eric, et al.
Publicado: (2025)

The Physics of Cometary Anti-tails as Observed in 3I/ATLAS
por: Keto, Eric, et al.
Publicado: (2025)

A Physical Model for the Ice Coma of the Interstellar, Hyperactive Comet 3I/ATLAS
por: Keto, Eric, et al.
Publicado: (2025)

Quasi-equilibrium chemical evolution in starless cores
por: Rawlings, Jonathan, et al.
Publicado: (2024)

Equilibrium Simplified Chemistries for H2O and CO in three-phase astrochemical models
por: Rawlings, Jonathan, et al.
Publicado: (2025)

Cosmic Ray Feedback on Bi-stable ISM Turbulence
por: Habegger, Roark, et al.
Publicado: (2024)

Galactic Dust Polarization in Turbulent Multiphase ISM: On the Origin of the $EE/BB$ Asymmetry
por: Hu, Yue, et al.
Publicado: (2026)

The Role of Pressure in the Structure and Stability of GMCs in the Andromeda Galaxy
por: Lada, C. J., et al.
Publicado: (2025)

The Arizona Molecular ISM Survey with the SMT: Survey Overview and Public Data Release
por: Keenan, Ryan P., et al.
Publicado: (2024)

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

Examining Turbulence in Galactic Molecular Clouds - II: Continuity of Turbulence Cascading in a Portion of the Local Arm
por: Ma, Yuehui, et al.
Publicado: (2025)

A JWST/MIRI View of the ISM in M83: I. Resolved Molecular Hydrogen Properties, Star Formation, and Feedback
por: Jones, Logan H., et al.
Publicado: (2024)

A New Framework for ISM Emission Line Models: Connecting Multi-Scale Simulations Across Cosmological Volumes
por: Yang, Shengqi, et al.
Publicado: (2024)

The molecular diversity of the ISM in galaxies across cosmic time
por: Bouvier, Mathilde, et al.
Publicado: (2025)

The Launching of Galactic Winds from a Multiphase ISM
por: Hidalgo-Pineda, Fernando, et al.
Publicado: (2025)

Direct measurement of ISM proper motion with image registration
por: Piecka, M., et al.
Publicado: (2025)

Supernova dust destruction in the magnetized turbulent ISM
por: Kirchschlager, Florian, et al.
Publicado: (2024)

The Arizona Molecular ISM Survey with the SMT: Variations in the CO(2-1)/CO(1-0) Line Ratio Across the Galaxy Population
por: Keenan, Ryan P., et al.
Publicado: (2024)

The Arizona Molecular ISM Survey with the SMT: The Diverse Carbon Monoxide Line Ratios and Spectral Line Energy Distributions of Star Forming Galaxies
por: Keenan, Ryan P., et al.
Publicado: (2025)

Effects of Radiative Transfer on the Observed Anisotropy in MHD Turbulent Molecular Simulations
por: Hernández-Padilla, D., et al.
Publicado: (2024)

MARTINI: Mock Array Radio Telescope Interferometry of the Neutral ISM
por: Oman, Kyle A.
Publicado: (2024)

AGN feedback in isolated galaxies with a SMUGGLE multiphase ISM
por: Sivasankaran, Aneesh, et al.
Publicado: (2024)

AGN feedback in merging galaxies with a SMUGGLE multiphase ISM
por: Sivasankaran, Aneesh, et al.
Publicado: (2025)

First Constraints on the ISM Conditions of a Low Mass, Highly Obscured z=4.27 Main Sequence Galaxy
por: Mizener, Andrew, et al.
Publicado: (2024)

3D ISM structure challenges the Serkowski relation
por: Mandarakas, Nikolaos, et al.
Publicado: (2024)

MHD lensing in inhomogeneous ISM for qualitative understanding of the morphology of supernova remnants
por: Sofue, Yoshiaki
Publicado: (2024)

Ram pressure stripping in clusters: Gravity can bind the ISM but not the CGM
por: Ghosh, Ritali, et al.
Publicado: (2024)

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)

Argon X-ray absorption in the local ISM
por: Gatuzz, E., et al.
Publicado: (2024)

Turbulent Pressure Heats Gas and Suppresses Star Formation in Galactic Bar Molecular Clouds
por: Nilipour, Andy, et al.
Publicado: (2024)

Examining Turbulence in Galactic Molecular Clouds -- I: A Statistical Analysis of Velocity Structures
por: Ma, Yuehui, et al.
Publicado: (2025)

CO spectra of the ISM in the Host Galaxies of the Most Luminous WISE-Selected AGNs
por: Martin, Lee R., et al.
Publicado: (2024)

The Emergence of Prebiotic Chemistry in the ISM
por: Jimenez-Serra, Izaskun, et al.
Publicado: (2025)

Where do stars explode in the ISM? -- The distribution of dense gas around evolved massive stars in M33
por: Sarbadhicary, Sumit K., et al.
Publicado: (2023)

The Rhythm of the ISM: Tracing the Timescales of Gas Evolution and Star Formation across Galactic Environments
por: Kocjan, Zuzanna, et al.
Publicado: (2026)

Mixing between AGN winds and ISM clouds produces luminous X-ray emission
por: Ward, Samuel Ruthven, et al.
Publicado: (2025)

Gas Phase Distribution in the Neutral ISM: A Comparison between Observation and Numerical Simulation
por: Koley, Atanu
Publicado: (2026)

Widespread Hot Molecular Gas Heated by Shear-induced Turbulence in the Galactic Center
por: Li, Juan, et al.
Publicado: (2025)