SPH simulations of grain growth in protoplanetary disks

Astronomy and Astrophysics

Volumn 487, Issue 1, 2008, Pages 265-270

  Laibe, G ^a,b,c,d   Gonzalez, J F ^a,b,c,d   Fouchet, L ^e   Maddison, S T ^f  

^a UNIVERSITÉ DE LYON   (France)

^b UNIVERSITÉ LYON 1   (France)

^c CENTRE DE RECHERCHE ASTROPHYSIQUE DE LYON   (France)

^d UNIVERSITÉ DE LYON   (France)

^e ETH ZURICH   (Switzerland)

^f SWINBURNE UNIVERSITY OF TECHNOLOGY   (Australia)

Author keywords

Hydrodynamics; Methods: numerical; Planetary systems: protoplanetary disks

Indexed keywords

BI MODAL DISTRIBUTION; DUST DISTRIBUTION; DUST DYNAMICS; EVOLUTION (CO); GRAIN SIZES; PILE UPS; PLANET FORMATION; PROTO-PLANETARY DISKS; RADIAL MIGRATION; SPATIAL DISTRIBUTION OF; SPH CODE;

AGGLOMERATION; AGRICULTURAL PRODUCTS; CODES (STANDARDS); CODES (SYMBOLS); DISKS (MACHINE COMPONENTS); DISKS (STRUCTURAL COMPONENTS); DUST; ECOLOGY; FLUID DYNAMICS; FLUID MECHANICS; GRAIN (AGRICULTURAL PRODUCT); GRAIN SIZE AND SHAPE; SIZE DISTRIBUTION; TWO PHASE FLOW;

GRAIN GROWTH;

EID: 48249088113     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:200809522     Document Type: Article

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