Experimental evidence for water formation on interstellar dust grains by hydrogen and oxygen atoms

Astronomy and Astrophysics

Volumn 512, Issue 5, 2010, Pages

  Dulieu, F ^a   Amiaud, L ^a   Congiu, E ^a   Fillion, J H ^a   Matar, E ^a   Momeni, A ^a   Pirronello, V ^b   Lemaire, J L ^a  

^a UNIVERSITÉ DE CERGY PONTOISE   (France)

^b UNIVERSITY OF CATANIA   (Italy)

Author keywords

Astrochemistry; Dust, extinction; ISM: molecules; Methods: laboratory; Molecular processes

Indexed keywords

CLOUDS; DEUTERIUM; DUST; HYDROGEN; OXYGEN; TEMPERATURE PROGRAMMED DESORPTION;

AMORPHOUS WATER; ASTROCHEMISTRY; COMPLEX CHEMISTRY; DUST , EXTINCTION; DUST GRAINS; EXPERIMENTAL EVIDENCE; GRAIN SURFACE; INTERSTELLAR CLOUDS; INTERSTELLAR DUST; INTERSTELLAR MEDIUMS; KEY PROCESS; METHODS: LABORATORY; MOLECULAR DIVERSITY; MOLECULAR PROCESS; OXYGEN ATOM; PRISTINE WATERS; WATER FORMATION; WATER ICE; WATER SYNTHESIS;

ATOMS;

EID: 77950414274     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200912079     Document Type: Article

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