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Volumn 606, Issue 2 I, 2004, Pages 983-987

On the importance of gas flow through porous bodies for the formation of planetesimals

Author keywords

Hydrodynamics; Planetary systems: protoplanetary disks; Planets and satellites: formation; Solar system: formation

Indexed keywords


EID: 2442474111     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/383122     Document Type: Article
Times cited : (26)

References (22)
  • 2
    • 0001184775 scopus 로고    scopus 로고
    • ed. V. Mannings, A. Boss, & S. S. Russell (Tucson: Univ. Arizona Press)
    • Beckwith, S. V. W., Henning, T., & Nakagawa, Y. 2000, in Protostars and Planets IV, ed. V. Mannings, A. Boss, & S. S. Russell (Tucson: Univ. Arizona Press), 533
    • (2000) Protostars and Planets IV , pp. 533
    • Beckwith, S.V.W.1    Henning, T.2    Nakagawa, Y.3
  • 11
  • 21
    • 0035475050 scopus 로고    scopus 로고
    • _. 2001b, Phys. Rev. E, 64, 046301
    • (2001) Phys. Rev. E , vol.64 , pp. 046301


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.