Metallicity of the massive protoplanets around HR 8799 If formed by gravitational instability

Icarus

Volumn 207, Issue 2, 2010, Pages 503-508

  Helled, R ^a   Bodenheimer, P ^b  

^a UNIVERSITY OF CALIFORNIA   (United States)

^b University of California Santa Cruz   (United States)

Author keywords

Abundances, Interiors; Accretion; Planetary formation; Planetesimals

Indexed keywords

EID: 77952581400     PISSN: 00191035     EISSN: 10902643     Source Type: Journal    
DOI: 10.1016/j.icarus.2009.11.023     Document Type: Article

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