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Volumn 725, Issue 1, 2010, Pages 1242-1251

The physics of protoplanetesimal dust agglomerates. V. multiple impacts of dusty agglomerates at velocities above the fragmentation threshold

Author keywords

Accretion; Accretion disks; Methods: laboratory; Planets and satellites: formation; Protoplanetary disks

Indexed keywords


EID: 78650016393     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1088/0004-637X/725/1/1242     Document Type: Article
Times cited : (61)

References (23)
  • 17
    • 0000303344 scopus 로고
    • ed. E. H. Levy & J. I. Lunine (Tucson, AZ: Univ. Arizona Press)
    • Weidenschilling, S. J., & Cuzzi, J. N. 1993, in Protostars and Planets III, ed. E. H. Levy & J. I. Lunine (Tucson, AZ: Univ. Arizona Press), 1031
    • (1993) Protostars and Planets III , pp. 1031
    • Weidenschilling, S.J.1    Cuzzi, J.N.2


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.