On the structure of the turbulent interstellar atomic hydrogen: II. First comparison between observation and theory. Are the characteristics of molecular clouds determined early in the turbulent 2-phase atomic gas?

Astronomy and Astrophysics

Volumn 465, Issue 2, 2007, Pages 445-456

  Hennebelle, P ^a   Audit, E ^b   Miville Deschenes M A ^c  

^a ECOLE NORMALE SUPÉRIEURE   (France)

^b DIF   (France)

^c UNIVERSITÉ PARIS SUD   (France)

Author keywords

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

Indexed keywords

CLOUDS; COMPUTER SIMULATION; DENSITY (SPECIFIC GRAVITY); HYDRODYNAMICS; HYDROGEN; STATISTICS;

ATOMIC GAS; COLUMN DENSITY; INSTABILITIES; MOLECULAR CLOUDS;

ASTROPHYSICS;

EID: 34147150672     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20066141     Document Type: Article

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