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Volumn 165, Issue 2, 2003, Pages 438-442

Radial drift of particles in the solar nebula: Implications for planetesimal formation

Author keywords

Planetesimals; Solar nebula

Indexed keywords


EID: 0141976806     PISSN: 00191035     EISSN: None     Source Type: Journal    
DOI: 10.1016/S0019-1035(03)00169-6     Document Type: Article
Times cited : (35)

References (10)
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  • 2
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  • 4
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    • Goodman, J.1    Pindor, B.2
  • 5
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  • 7
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    • Evolution of the Protoplanetary Cloud and Formation of the Earth and Planets
    • Nauka, Moscow
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    • Safronov, V.S.1
  • 8
    • 0042161238 scopus 로고
    • Can gravitational instability form planetesimals?
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    • Weidenschilling, S.J.1
  • 9
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  • 10
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    • Planetesimal formation by gravitational instability
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    • Youdin, A.N.1    Shu, F.H.2


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.