Warm non-equilibrium gas phase chemistry as a possible origin of high HDO/H2O ratios in hot and dense gases: Application to inner protoplanetary discs

Monthly Notices of the Royal Astronomical Society

Volumn 407, Issue 1, 2010, Pages 232-246

  Thi, W F ^a   Woitke, P ^b   Kamp, I ^c  

^a UNIVERSITY OF EDINBURGH   (United Kingdom)

^b UK ASTRONOMY TECHNOLOGY CENTRE   (United Kingdom)

^c UNIVERSITY OF GRONINGEN   (Netherlands)

Author keywords

Astrochemistry

Indexed keywords

ACTIVATION ENERGY; CHEMICAL ANALYSIS; COMETS; DEUTERIUM; DUST; SILICATES; SURFACE CHEMISTRY;

ASTROCHEMISTRY; DENSE GAS; DRY EARTHS; GAS PHASE CHEMISTRY; HOT GAS; HYDRATED SILICATE; LOW GAS TEMPERATURE; NON EQUILIBRIUM; PROTOPLANETARY DISKS; WATER ICE;

GASES;

EID: 77956398674     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2009.16162.x     Document Type: Article

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