On the structure of the turbulent interstellar atomic hydrogen: I. Physical characteristics. Influence and nature of turbulence in a thermally bistable flow

Astronomy and Astrophysics

Volumn 465, Issue 2, 2007, Pages 431-443

  Hennebelle, P ^a   Audit, E ^b  

^a ECOLE NORMALE SUPÉRIEURE   (France)

^b CEA SACLAY   (France)

Author keywords

Hydrodynamics; Instabilities; ISM: clouds; ISM: kinematics and dynamics; ISM: structure

Indexed keywords

CLOUDS; HYDRODYNAMICS; HYDROGEN; STATISTICAL METHODS; TURBULENCE; TURBULENT FLOW;

HIGH RESOLUTION BIDIMENSIONAL NUMERICAL SIMULATIONS; INSTABILITIES; STATISTICAL PROPERTIES; TURBULENT INTERSTELLAR ATOMIC HYDROGEN;

ASTROPHYSICS;

EID: 34147108100     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20066139     Document Type: Article

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