Dissipative structures of diffuse molecular gas I. Broad HCO+ (J= 1-0) emission

Astronomy and Astrophysics

Volumn 452, Issue 2, 2006, Pages 511-522

  Falgarone, E ^a   Pineau Des Forets G ^b,c   Hily Blant, P ^d   Schilke, P ^e  

^a ECOLE NORMALE SUPÉRIEURE   (France)

^b UNIVERSITÉ PARIS SUD   (France)

^c OBSERVATOIRE DE PARIS   (France)

^d IRAM   (France)

^e MAX PLANCK INSTITUT FÜR RADIOASTRONOMIE   (Germany)

Author keywords

Astrochemistry; ISM: kinematics and dynamics; ISM: molecules; ISM: structure; Radio lines: ISM; Turbulence

Indexed keywords

ELECTROMAGNETIC WAVE EMISSION; ENERGY DISSIPATION; KINEMATICS; PHOTONS; SIGNAL TO NOISE RATIO; STATISTICAL METHODS; TURBULENCE; ULTRAVIOLET RADIATION;

CHEMICAL RELAXATION PHASE; DIFFUSE MOLECULAR CLOUDS; MOLECULAR GAS; SWAS SATELLITE;

ASTROPHYSICS;

EID: 33744950686     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20054087     Document Type: Article

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