High-mass, four-planet configurations for HR 8799: Constraining the orbital inclination and age of the system

Astrophysical Journal

Volumn 755, Issue 1, 2012, Pages

  Sudol, Jeffrey J ^a   Haghighipour, Nader ^b  

^a WEST CHESTER UNIVERSITY   (United States)

^b UNIVERSITY OF HAWAII   (United States)

Author keywords

planets and satellites: dynamical evolution and stability; stars: individual (HR 8799)

Indexed keywords

EID: 84864459395     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1088/0004-637X/755/1/38     Document Type: Article

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