International audience
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August 1, 2014 (v1)Conference paperUploaded on: December 3, 2022
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June 10, 2018 (v1)Conference paper
International audience
Uploaded on: December 3, 2022 -
June 25, 2008 (v1)Publication
Context: The main sequence binary star 61 Cyg (K5V+K7V) is our nearest stellar neighbour in the northern hemisphere. This proximity makes it a particularly well suited system for very high accuracy interferometric radius measurements. Aims: Our goal is to constrain the poorly known evolutionary status and age of this bright binary star....
Uploaded on: December 4, 2022 -
December 14, 2020 (v1)Conference paper
International audience
Uploaded on: December 3, 2022 -
December 14, 2020 (v1)Conference paper
The CHARA Array is the longest baseline optical interferometer in the world. Operated with natural seeing, it has delivered landmark sub-milliarcsecond results in the areas of stellar imaging, binaries, and stellar diameters. However, to achieve ambitious observations of faint targets such as young stellar objects and active galactic nuclei,...
Uploaded on: February 22, 2023 -
December 14, 2020 (v1)Conference paper
The CHARA Array is the longest baseline optical interferometer in the world. Operated with natural seeing, it has delivered landmark sub-milliarcsecond results in the areas of stellar imaging, binaries, and stellar diameters. However, to achieve ambitious observations of faint targets such as young stellar objects and active galactic nuclei,...
Uploaded on: December 4, 2022