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Astrophysical Journal

Volumn 701, Issue 1, 2009, Pages 130-141

The physics of protoplanetesimal dust agglomerates. IV. toward a dynamical collision model

(5) Guttler C a Krause, M a Geretshauser, R J b Speith, R b Blum, J a

a TECHNICAL UNIVERSITY OF BRAUNSCHWEIG (Germany)

b UNIVERSITY OF TÜBINGEN (Germany)

Author keywords

Accretion, accretion disks; Methods: Laboratory; Methods: Numerical; Planetary systems: Formation solar system: Formation

Indexed keywords

EID: 70449591680 PISSN: 0004637X EISSN: 15384357 Source Type: Journal
DOI: 10.1088/0004-637X/701/1/130 Document Type: Article

Times cited : (125)

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