Dust coagulation and fragmentation in molecular clouds I. How collisions between dust aggregates alter the dust size distribution

Astronomy and Astrophysics

Volumn 502, Issue 3, 2009, Pages 845-869

  Ormel, C W ^a,b   Paszun, D ^c   Dominik, C ^c,d   Tielens, A G G M ^e,f  

^a UNIVERSITY OF GRONINGEN   (Netherlands)

^b MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

^c UNIVERSITY OF AMSTERDAM   (Netherlands)

^d RADBOUD UNIVERSITY NIJMEGEN   (Netherlands)

^e NASA AMES RESEARCH CENTER   (United States)

^f LEIDEN UNIVERSITY   (Netherlands)

Author keywords

Extinction; ISM: Clouds; ISM: Dust; Methods: Numerical; Turbulence

Indexed keywords

BINARY MODELS; COAGULATION MODELS; COLLISION VELOCITY; COLLISIONAL EVOLUTION; DUST GRAINS; DUST SIZE DISTRIBUTION; EVOLUTION MODELS; EXTINCTION; GAS DENSITY; INTERNAL STRUCTURE; INTERSTELLAR MEDIUMS; ISM: CLOUDS; ISM: DUST; MASS DISTRIBUTION; MASS SPECTRA; MATERIAL PROPERTY; METHODS: NUMERICAL; MOLECULAR CLOUDS; PARAMETER STUDIES; STEADY STATE; SUPPORT MECHANISM; TIME-SCALES; TWO STAGE;

CLOUDS; COAGULATION; DENSITY OF GASES; MASS SPECTROMETRY; NUMERICAL METHODS; SIZE DISTRIBUTION; TURBULENCE;

DUST;

EID: 68649103261     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200811158     Document Type: Article

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