A combined subaru/VLT/MMT 1-5 μm study of planets orbiting HR 8799: Implications for atmospheric properties, masses, and formation

Astrophysical Journal

Volumn 729, Issue 2, 2011, Pages

  Currie, Thayne ^a   Burrows, Adam ^b   Itoh, Yoichi ^c   Matsumura, Soko ^d   Fukagawa, Misato ^e   Apai, Daniel ^f   Madhusudhan, Nikku ^b   Hinz, Philip M ^g   Rodigas, T J ^g   Kasper, Markus ^h   Pyo, T S ⁱ   Ogino, Satoshi ^c  

^a NASA GODDARD SPACE FLIGHT CENTER   (United States)

^b PRINCETON UNIVERSITY   (United States)

^c KOBE UNIVERSITY   (Japan)

^d Bldg 142   (United States)

^e OSAKA UNIVERSITY   (Japan)

^f STScI   (United States)

^g UNIVERSITY OF ARIZONA   (United States)

^h EUROPEAN SOUTHERN OBSERVATORY   (Germany)

ⁱ NATIONAL ASTRONOMICAL OBSERVATORY OF JAPAN   (Japan)

Author keywords

brown dwarfs; instrumentation: adaptive optics; planetary systems; stars: individual (HR 8799); techniques: image processing

Indexed keywords

EID: 79952154607     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1088/0004-637X/729/2/128     Document Type: Article

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