On the structure of the turbulent interstellar clouds . Influence of the equation of state on the dynamics of 3D compressible flows

2009/11/04 by E. Audit, P. Hennebelle · 3 citations
Chemical Engineering · Physics and Astronomy · #Advanced Combustion Engine Technologies #Astro and Planetary Science #Astrophysics #Astrophysics and Star Formation Studies #Barotropic fluid #Context (archaeology) #Galaxy #Interstellar medium #Mechanics #Molecular cloud #Physics #Polytropic process #Power law #Star formation #Stars #Statistical physics #Statistics #Stellar, planetary, and galactic studies #Turbulence #Velocity dispersion #astro-ph.GA

paper · pdf · doi:10.1051/0004-6361/200912695

accepted for publication to A&A

arxiv created 2009/11/04 · openalex publication_date 2010/01/01 · arxiv updated 2015/05/14 · openalex created_date 2016/06/24 · openalex updated_date 2026/07/22

Abstract

International audience

Citations

• Turbulence measurements from Hi absorption spectra
• Cosmic-Ray Heating of the Interstellar Gas
• Structure and Stability of Phase Transition Layers in the Interstellar Medium
• H I in the Galaxy
• Influence of Alfvén waves on thermal instability in the interstellar medium

Cited by

• Turbulent molecular clouds
• Feeding versus Falling: The Growth and Collapse of Molecular Clouds in a Turbulent Interstellar Medium
• The sonic scale of interstellar turbulence