Does the gas flow through a porous dust aggregate help its growth in a protoplanetary disk?

Icarus

Volumn 176, Issue 1, 2005, Pages 220-223

  Sekiya, Minoru ^a   Takeda, Hidenori ^b  

^a KYUSHU UNIVERSITY   (Japan)

^b KYOTO UNIVERSITY   (Japan)

Author keywords

Planetary formation; Planetesimals

Indexed keywords

EID: 18844401143     PISSN: 00191035     EISSN: None     Source Type: Journal    
DOI: 10.1016/j.icarus.2005.01.008     Document Type: Article

References (25)

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