From the warm magnetized atomic medium to molecular clouds

2008/05/09 by P. Hennebelle, R. Banerjee, Robi Banerjee +5 · 1 citation
Physics and Astronomy · #Astrobiology #Astrophysics #Astrophysics and Star Formation Studies #Atomic physics #Chemical physics #Cold Atom Physics and Bose-Einstein Condensates #Context (archaeology) #Geology #Materials science #Mechanics #Molecular cloud #Paleontology #Physics #Quantum, superfluid, helium dynamics #Transonic #astro-ph

paper · pdf · doi:10.1051/0004-6361:200810165

submitted to A&A

arxiv created 2008/05/09 · openalex publication_date 2008/06/24 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

Context. It has been proposed that giant molecular complexes form at the sites of streams of diffuse warm atomic gas that collide at transonic velocities.

Citations

• FLASH: An Adaptive Mesh Hydrodynamics Code for Modeling Astrophysical Thermonuclear Flashes
• Formation of Structure in Molecular Clouds: A Case Study

Cited by

• Linked Evolution of Gas and Star Formation in Galaxies Over Cosmic History