THE chara array angular diameter of HR 8799 favors planetary masses for its imaged companions

Astrophysical Journal

Volumn 761, Issue 1, 2012, Pages

  Baines, Ellyn K ^a   White, Russel J ^b   Huber, Daniel ^c   Jones, Jeremy ^b   Boyajian, Tabetha ^b   McAlister, Harold A ^b   Ten Brummelaar, Theo A ^b   Turner, Nils H ^b   Sturmann, Judit ^b   Sturmann, Laszlo ^b   Goldfinger, P J ^b   Farrington, Christopher D ^b   Riedel, Adric R ^b   Ireland, Michael ^d   Von Braun, Kaspar ^e   Ridgway, Stephen T ^f  

^a NAVAL RESEARCH LABORATORY   (United States)

^b GEORGIA STATE UNIVERSITY   (United States)

^c NASA AMES RESEARCH CENTER   (United States)

^d MACQUARIE UNIVERSITY   (Australia)

^e CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^f KITT PEAK NATIONAL OBSERVATORY   (United States)

Author keywords

planetary systems; stars: fundamental parameters; stars: individual (HR 8799); techniques: high angular resolution; techniques: interferometric

Indexed keywords

EID: 84870337805     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1088/0004-637X/761/1/57     Document Type: Article

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