Observation of double star by long-baseline interferometry

Abstract

This paper serves as a reference on how to estimate the parameters of binary stars and how to combine multiple techniques, namely astrometry, interferometry and radial velocities.

F. Millour, A. Chiavassa, L. Bigot, O. Chesneau, A. Meilland \& P. Stee. What can the highest angular resolution bring to stellar astrophysics?, 69-70, EDP sciences, 2015, EAS publication series, 978-2-7598-1833-4. \<10.1051/eas/1569020\>. \<http://www.eas-journal.org/articles/eas/abs/2014/04/contents/contents.html\&gt

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• Binary interaction dominates the evolution of massive stars
• First Resolved Images of the Eclipsing and Interacting Binary Beta Lyrae
• Direct constraint on the distance of y2 Velorum from AMBER/VLTI observations
• The Expanding Fireball of Nova Delphini 2013
• VLTI/AMBER interferometric observations of the recurrent Nova RS Oph 5.5 days after outburst
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Cited by in corpus (2)

• ARMADA I: Triple Companions Detected in B-Type Binaries alpha Del and nu Gem
• ARMADA II: Further Detections of Inner Companions to Intermediate Mass Binaries with Micro-Arcsecond Astrometry at CHARA and VLTI