2 papers
astro-ph.SR2018
WASP 0639-32: a new F-type subgiant/K-type main-sequence detached eclipsing binary from the WASP project
J. A. Kirkby-Kent, P. F. L. Maxted, A. M. Serenelli +3
Abridged. Our aim is to measure the masses and radii of the stars in a newly-discovered detached eclipsing binary system to a high precision (1%), enabling the system to b…
astro-ph.SR2016
Absolute parameters for AI Phoenicis using WASP photometry
J. A. Kirkby-Kent, P. F. L. Maxted, A. M. Serenelli +5
AI Phe is a double-lined, detached binary, in which a K-type sub-giant star totally eclipses its main-sequence companion every 24.6 days. This configuration makes AI Phe ideal for…