When sticking influences H2 formation

Astronomy and Astrophysics

Volumn 535, Issue , 2011, Pages

  Cazaux, S ^a   Morisset, S ^b   Spaans, M ^a   Allouche, A ^b  

^a UNIVERSITY OF GRONINGEN   (Netherlands)

^b CNRS   (France)

Author keywords

astrochemistry; ISM: abundances; ISM: molecules; molecular processes

Indexed keywords

ASTROCHEMISTRY; CATALYTIC PROPERTIES; CLASSICAL-QUANTUM; DENSITY FUNCTIONAL THEORY CALCULATIONS; DUST GRAINS; DUST SURFACE; EARLY UNIVERSE; GAS TEMPERATURE; GASPHASE; HIGH ENERGY; INTERSTELLAR DUST; ISM: ABUNDANCE; ISM: MOLECULES; KINETIC MONTE CARLO SIMULATION; MOLECULAR HYDROGEN; MOLECULAR PROCESS; ORDERS OF MAGNITUDE; PHOTON-DOMINATED REGIONS; PHYSISORBED; STICKING COEFFICIENTS; STICKING PROBABILITY; VIBRATIONAL MODES;

CHEMISORPTION; COMPUTER SIMULATION; DENSITY FUNCTIONAL THEORY; DUST; HYDROGEN; MOLECULAR PHYSICS; MONTE CARLO METHODS; QUANTUM THEORY;

ATOMS;

EID: 80555133131     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201117220     Document Type: Article

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