Beyond the pseudo-time-dependent approach: Chemical models of dense core precursors

Astronomy and Astrophysics

Volumn 515, Issue 8, 2010, Pages

  Hassel, G E ^a   Herbst, E ^a   Bergin, E A ^b  

^a OHIO STATE UNIVERSITY   (United States)

^b UNIVERSITY OF MICHIGAN   (United States)

Author keywords

Evolution; ISM: clouds; ISM: molecules; Shock waves; Stars: formation

Indexed keywords

CLOUDS; COMPUTER SIMULATION; GASES; MODELS; MOLECULAR BIOLOGY; MOLECULES; SHOCK WAVES; STARS;

CHEMICAL MODEL; CHEMICAL NETWORKS; CORE FORMATION; DENSE CORE; DIFFUSE INTERSTELLAR MEDIUMS; EVOLUTION; GAS PHASE MOLECULES; GASPHASE; HYDRODYNAMIC SHOCK; INITIAL CONDITIONS; ISM : CLOUDS; MOLECULAR EVOLUTION; MOLECULAR GAS; MOLECULAR HYDROGEN; MOLECULAR ICES; PHYSICAL CONDITIONS; SHOCK PHASE; STARS: FORMATION; SURFACE MECHANISM; TIME-DEPENDENT; WATER ICE; WAVE SIMULATIONS;

ICE;

EID: 77953376318     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200913896     Document Type: Article

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