The outcome of protoplanetary dust growth: pebbles, boulders, or planetesimals?: I. Mapping the zoo of laboratory collision experiments

Astronomy and Astrophysics

Volumn 513, Issue 11, 2010, Pages

  Zsom, A ^a   Ormel, C W ^a   Guttler C ^b   Blum, J ^b   Dullemond, C P ^a  

^a MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

^b TECHNICAL UNIVERSITY OF BRAUNSCHWEIG   (Germany)

Author keywords

Accretion; Accretion disks; Methods: numerical; Planets and satellites: formation

Indexed keywords

AGGREGATES; DENSITY OF GASES; DISTRIBUTION FUNCTIONS; MONTE CARLO METHODS; NUMERICAL METHODS; PLANETS; SATELLITES; TURBULENCE;

ACCRETION; ACCRETION DISKS; CATASTROPHIC FRAGMENTATION; CONTINUOUS TRANSITIONS; LABORATORY EXPERIMENTS; MAXIMUM AGGREGATE SIZES; METHODS: NUMERICALS; PLANETS AND SATELLITES: FORMATION;

DUST;

EID: 77951771137     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200912976     Document Type: Article

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