Molecular hydrogen formation during dense interstellar cloud collapse

Monthly Notices of the Royal Astronomical Society

Volumn 361, Issue 2, 2005, Pages 550-558

  Acharyya, Kinsuk ^a   Chakrabarti, Sandip K ^a,b   Chakrabarti, Sonali ^a,c  

^a INDIAN CENTRE FOR SPACE PHYSICS   (India)

^b S N BOSE NATIONAL CENTRE FOR BASIC SCIENCES   (India)

^c Maharaja Manindra Chandra College   (India)

Author keywords

ISM: Atoms; ISM: Clouds; ISM: Evolution; ISM: Molecules

Indexed keywords

AMORPHOUS CARBON; HYDROGEN; OLIVINE;

GAS-PHASES; GRAIN SURFACE; HIGHEST TEMPERATURE; INTERSTELLAR CLOUDS; ISM : CLOUDS; ISM: ATOMS; ISM:EVOLUTION; ISM:MOLECULES; MOLECULAR HYDROGEN; RATE EQUATIONS;

MOLECULES;

EID: 23444455481     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2005.09195.x     Document Type: Article

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