A&A 601, A34 (2017) Astronomy DOI: 10.1051/0004-6361/201629260 & c ESO 2017 Astrophysics Resolved astrometric orbits of ten O-type binaries?,?? J.-B. Le Bouquin1, H. Sana2, E. Gosset3,???, M. De Becker3, G. Duvert1, O. Absil3,????, F. Anthonioz1, J.-P. Berger4, S. Ertel11, R. Grellmann8, S. Guieu1; 7, P. Kervella5; 6, M. Rabus9; 11, and M. Willson10 1 Univ. Grenoble Alpes, CNRS, IPAG, 38000 Grenoble, France e-mail:
[email protected] 2 Institute of Astrophysics, KU Leuven, Celestijnlaan 200D, 3001 Leuven, Belgium 3 Space sciences, Technologies and Astrophysics Research (STAR) Institute, Université de Liège, 19C Allée du Six Août, 4000 Liège, Belgium 4 European Southern Observatory, Schwarzschild-Str. 2, 85748 Garching bei München, Germany 5 Unidad Mixta Internacional Franco-Chilena de Astronomía (UMI 3386), CNRS/INSU France; Departamento de Astronomía, Universidad de Chile, Camino El Observatorio 1515, Las Condes, Santiago, Chile 6 LESIA, UMR 8109, Observatoire de Paris, CNRS, UPMC, Univ. Paris-Diderot, PSL, 5 place Jules Janssen, 92195 Meudon, France 7 European Southern Observatory, Alonso de Cordova 3107, Vitacura, 19001 Casilla, Santiago 19, Chile 8 I. physikalisches Institut, Universität zu Köln, Zülpicherstr. 77, 50937 Köln, Germany 9 Instituto de Astrofisica, Facultad de Fisica, Pontificia Universidad Católica de Chile, Casilla 306, 22 Santiago, Chile 10 University of Exeter, Astrophysics Group, School of Physics, Stocker Road, Exeter EX4 4QL, UK 11 Max Planck Institute for Astronomy, Königstuhl 17, 69117 Heidelberg, Germany Received 7 July 2016 / Accepted 23 July 2016 ABSTRACT Aims. Our long-term aim is to derive model-independent stellar masses and distances for long period massive binaries by combining apparent astrometric orbit with double-lined radial velocity amplitudes (SB2).