Molecular absorption lines toward star-forming regions: A comparative study of HCO+, HNC, HCN, and CN

Astronomy and Astrophysics

Volumn 520, Issue 20, 2010, Pages

  Godard, B ^a,b   Falgarone, E ^a   Gerin, M ^a   Hily Blant, P ^c   De Luca, M ^a  

^a OBSERVATOIRE DE PARIS   (France)

^b UNIVERSITÉ PARIS SUD   (France)

^c UNIV GRENOBLE ALPES   (France)

Author keywords

astrochemistry; ISM: clouds; ISM: kinematics and dynamics; ISM: molecules; ISM: structure; turbulence

Indexed keywords

ASTROCHEMISTRY; ISM : CLOUDS; ISM: KINEMATICS AND DYNAMICS; ISM: MOLECULES; ISM: STRUCTURE;

BEARINGS (STRUCTURAL); CHEMICAL PROPERTIES; CLOUDS; GAS ABSORPTION; GASES; KINEMATICS; MOLECULAR STRUCTURE; MOLECULES; PHASE EQUILIBRIA; TURBULENCE; VELOCITY;

GAS FUEL PURIFICATION;

EID: 78649258458     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201014283     Document Type: Article

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