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MOLECULAR CLOUDS IN GALAXIES WITH DIFFERENT Z: FRAGMENTATION OF DIFFUSE CLOUDS DRIVEN BY OPACITY.
Publications of the Astronomical Society of the Pacific, 1986Molecular clouds are formed from diffuse interstellar clouds when the external ultraviolet radiation field is prevented from penetrating into the cloud. The opacity is provided mainly by dust grains and the required column density to the cloud center is larger than about 5 x 10 to the 20th (solar Z/Z)/sq cm.
Jose Franco, Donald P. Cox
exaly +2 more sources
MHD Shock Waves in Diffuse Molecular Clouds
1987The theory of low-velocity (v s ≤ 30km/s) MHD shock waves in diffuse molecular gas is reviewed. The multifluid nature of the gas dynamics is emphasized, and the important microphysics and chemistry is mentioned. Recent attempts to use shock waves to account for the abundance of interstellar CH+ are discussed, and the required shock frequency and global
openaire +1 more source
Extragalactic molecular clouds and chemistry of diffuse interstellar clouds
2009openaire +1 more source
Improving Outcomes for Patients with Diffuse Large B-cell Lymphoma†
Ca-A Cancer Journal for Clinicians, 2010Christopher R Flowers +2 more
exaly
THE CHEMISTRY OF INTERSTELLAR ARGONIUM AND OTHER PROBES OF THE MOLECULAR FRACTION IN DIFFUSE CLOUDS
Astrophysical Journal, 2016David Neufeld, Mark Wolfire
exaly
Evolution and Emission of Cold, Warm and Hot Dust Populations in Diffuse and Molecular Clouds
Astrophysics and Space Science Library, 1996J Mayo Greenberg
exaly
Origin of CH+ in diffuse molecular clouds
Astronomy and Astrophysics, 2017Patrick Hennebelle +2 more
exaly
The role of clouds in improving the regression model for hourly values of diffuse solar radiation
Applied Energy, 2012Amauri Pereira de Oliveira +2 more
exaly
ON THE ORTHO:PARA RATIO OF H+3 IN DIFFUSE MOLECULAR CLOUDS*
Astrophysical Journal, 2011Kyle N Crabtree +2 more
exaly