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

Astronomy and Astrophysics

Volumn 511, Issue 1, 2010, Pages

  Audit, E ^a   Hennebelle, P ^b  

^a CEA SACLAY   (France)

^b OBSERVATOIRE DE PARIS   (France)

Author keywords

Instabilities; ISM: clouds; ISM: structure; Turbulence

Indexed keywords

3-DIMENSIONAL; ATOMIC HYDROGEN; BAROTROPIC; BISTABLES; BUILDING BLOCKES; EQUATION OF STATE; HIGH RESOLUTION; INSTABILITIES; INTERNAL VELOCITY; INTERSTELLAR CLOUDS; ISM : CLOUDS; ISM: STRUCTURE; MASS SPECTRA; MOLECULAR CLOUDS; NUMBER DENSITY; PHASE FLOW; POWER LAW; STATISTICAL PROPERTIES; THERMAL STRUCTURE; VELOCITY DISPERSION;

CLOUD COMPUTING; DISPERSIONS; DISTRIBUTION FUNCTIONS; EQUATIONS OF STATE; HYDROGEN; MASS SPECTROMETERS; MASS SPECTROMETRY; PROBABILITY DENSITY FUNCTION; RADIO ASTRONOMY; TURBULENCE;

CLOUDS;

EID: 79952822835     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200912695     Document Type: Article

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