The programme: Accurate masses for double-lined spectroscopic binary components

Y. Lebreton (1, 2) , J.-L. Halbwachs (3) , F. Kiefer (4) , F. Arenou (5) , B. Famaey (3) , P. Guillout (3) , R. Ibata (3) , T. Mazeh (6) , A. Nebot Gomez-Moran (3) , D. Pourbaix (7)

1 LESIA (UMR_8109) - Laboratoire d'études spatiales et d'instrumentation en astrophysique
2 IPR - Institut de Physique de Rennes
3 ObAS - Observatoire astronomique de Strasbourg
4 LGeco - Laboratoire de Génie de la Conception
5 GEPI - Galaxies, Etoiles, Physique, Instrumentation
6 TAU - School of Physics and Astronomy [Tel Aviv]
7 ULB - Université libre de Bruxelles

We present the programme: Accurate masses for double-lined spectroscopic binary components that combines spectroscopic and interferometric observations of binary stars which constitute a set of benchmarks for the analysis of the observations of several spatial missions (Gaia, TESS, PLATO).

Keywords: binaries: spectroscopic; binaries: visual; Astrometry

Domains: Sciences of the Universe [physics]; Sciences of the Universe [physics]; Astrophysics [astro-ph]; Sciences of the Universe [physics]; Astrophysics [astro-ph]; Solar and Stellar Astrophysics [astro-ph.SR]

Y. Lebreton, J.-L. Halbwachs, F. Kiefer, F. Arenou, B. Famaey, et al.. The programme: Accurate masses for double-lined spectroscopic binary components. PLATO STESCI WORKshop ii, May 2018, Milazzo, Italy. ⟨hal-02355535⟩