The importance of the ortho:para H 2 ratio for the deuteration of molecules during pre-protostellar collapse

Astronomy and Astrophysics

Volumn 449, Issue 2, 2006, Pages 621-629

  Flower, D R ^a   Pineau Des Forets G ^b,c   Walmsley, C M ^d  

^a DURHAM UNIVERSITY   (United Kingdom)

^b UNIVERSITÉ PARIS SUD   (France)

^c UNIVERSITÉ PARIS SACLAY   (France)

^d INAF OSSERVATORIO ASTROFISICO DI ARCETRI   (Italy)

Author keywords

Astrochemistry; ISM: molecules; Stars: formation; Submillimeter

Indexed keywords

ASTROCHEMISTRY; ISM: MOLECULES; STARS: FORMATION; SUBMILLIMETER;

DEUTERIUM; GRAVITATIONAL EFFECTS; HYDROGEN; IONS; NUCLEAR PHYSICS; REACTION KINETICS;

SPACE RESEARCH;

EID: 33645671836     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20054246     Document Type: Article

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