| Issue |
EAS Publications Series
Volume 69-70, 2014
What the Highest Angular Resolution Can Bring to Stellar Astrophysics?
|
|
|---|---|---|
| Page(s) | 335 - 372 | |
| Section | Multiple Stars | |
| DOI | https://doi.org/10.1051/eas/1569020 | |
| Published online | 10 September 2015 | |
What the Highest Angular Resolution Can Bring to Stellar Astrophysics?
F. Millour, A. Chiavassa, L. Bigot, O. Chesneau, A. Meilland and Ph. Stee (eds)
EAS Publications Series, 69–70 (2014) 335-372
F. Millour, A. Chiavassa, L. Bigot, O. Chesneau, A. Meilland and Ph. Stee (eds)
EAS Publications Series, 69–70 (2014) 335-372
Observation of Double Star by Long Baseline Interferometry
Laboratoire Lagrange, UMR 7293, Université de Nice Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, Bd. de l'Observatoire, 06304 Nice, France
e-mail: fmillour@oca.eu
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.
© EAS, EDP Sciences, 2015