CHARA Array Measurements of the Angular Diameters of Exoplanet Host Stars

Ellyn K. Baines; Harold A. McAlister; Theo A. ten Brummelaar; Nils H. Turner; Judit Sturmann; Laszlo Sturmann; P. J. Goldfinger; Stephen T. Ridgway

doi:10.1086/588009

arXiv · 0803.1411

CHARA Array Measurements of the Angular Diameters of Exoplanet Host Stars

Ellyn K. Baines·Harold A. McAlister·Theo A. ten Brummelaar·Nils H. Turner·Judit Sturmann·Laszlo Sturmann·P. J. Goldfinger·Stephen T. Ridgway

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Abstract

We have measured the angular diameters for a sample of 24 exoplanet host stars using Georgia State University's CHARA Array interferometer. We use these improved angular diameters together with Hipparcos parallax measurements to derive linear radii and to estimate the stars' evolutionary states.

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BibTeX RIS

Ellyn K. Baines, Harold A. McAlister, Theo A. ten Brummelaar, Nils H. Turner, Judit Sturmann, Laszlo Sturmann, P. J. Goldfinger, Stephen T. Ridgway. 2008-03-10. CHARA Array Measurements of the Angular Diameters of Exoplanet Host Stars. https://doi.org/10.1086/588009

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