Why HOC+ is detectable in interstellar clouds: The rate of the reaction between HOC+ and H2

Astrophysical Journal

Volumn 463, Issue 2 PART II, 1996, Pages

  Herbst, Eric ^a   Woon, David E ^b  

^a OHIO STATE UNIVERSITY   (United States)

^b MOLECULAR RESEARCH INSTITUTE   (United States)

Author keywords

ISM: abundances; ISM: clouds; ISM: molecules; Molecular processes

Indexed keywords

HYDROCARBON; HYDROGEN; ION;

ALGORITHM; ARTICLE; ASTRONOMY; CHEMICAL MODEL; CHEMISTRY; COMPUTER SIMULATION; ISOMERISM; MICROCLIMATE; NASA DISCIPLINE EXOBIOLOGY; NON-NASA CENTER; TEMPERATURE;

NASA DISCIPLINE EXOBIOLOGY; NON-NASA CENTER;

ALGORITHMS; ASTRONOMY; COMPUTER SIMULATION; EXTRATERRESTRIAL ENVIRONMENT; HYDROCARBONS; HYDROGEN; IONS; ISOMERISM; MODELS, CHEMICAL; TEMPERATURE;

EID: 0030153625     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/310059     Document Type: Article

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