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The CHARA array angular diameter of HR 8799 favors planetary masses for its imaged companions

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Date

2012

Authors

Baines, Ellyn K
White, Russel J
Huber, D
Jones, Jeremy
Boyajian, T S
McAlister, H
ten Brummelar, T
Turner, Nils
Sturmann, J
Goldfinger, P J

Journal Title

Journal ISSN

Volume Title

Publisher

IOP Publishing

Abstract

HR 8799 is an hF0 mA5 γ Doradus-, λ Bootis-, Vega-type star best known for hosting four directly imaged candidate planetary companions. Using the CHARA Array interferometer, we measure HR 8799's limb-darkened angular diameter to be 0.342 ± 0.008 mas (a

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Keywords

Citation

URI

http://hdl.handle.net/1885/66626

Collections

Open Access Research

Source

Astrophysical Journal, The

Type

Journal article

Book Title

Entity type

Access Statement

License Rights

DOI

10.1088/0004-637X/761/1/57

Restricted until

2037-12-31

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01_Baines_The_CHARA_array_angular_2012.pdf (2.27 MB)

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