Latest Articles for Gas Dynamics

Active galaxies significantly influence their surroundings through metal enrichment processes.

Research reveals how outflows shape star formation.

This study compares models of the circumgalactic medium to improve understanding of galaxies.

A new method enhances predictions for complex distributions using moment closure.

Research links solar active regions to gas flow patterns on the Sun's surface.

A look into the process of high-mass star formation and key influences.

This article examines gas movement in protoplanetary discs and its implications for hidden companions.

This article explores how gases evolve from polynomial to Gaussian distributions over time.

Examining how dust and gas interactions lead to planetesimal formation.

Study reveals how gas clouds collide to form dense regions for star formation.

Examining how misaligned disks behave around black holes and their implications.

Research reveals how gas molecules transfer energy during high-temperature events.

Exploring how celestial bodies repel each other in gas-filled disks.

The DIISC Survey studies gas behaviors around galaxies to enhance our understanding of galaxy evolution.

Unraveling the mysteries of one-dimensional gases through density correlations.

A look at gas transport and the impact on fuel cell efficiency.

Discover how hub-filament systems contribute to the birth of high-mass stars.

How gas clouds become stars reveals cosmic secrets.

This article explores the application of IMEX-RK methods in gas dynamics.

Discover how supernova remnants interact with cold gas clouds in space.

A look at how gas outflows shape star formation.

Examining how accretion disks evolve under gravitational and magnetic influences.

Learn how the nonlinear Boltzmann equation reveals gas particle behavior.

We improve simulations of binary star systems and their interacting disks.

MOGLI enables better understanding of multiphase gas in astrophysics.

Explore how collision integrals reveal the dynamics of dense gases.