http://iopscience.iop.org/0067-0049/215/1/15/ - Copyright The American Astronomical Society (AAS) and IOP Publishing Limited 2013
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Abstract :
[en] Multiplicity is one of the most fundamental observable properties of massive O-type stars and offers a promising way to discriminate between massive star formation theories. Nevertheless, companions at separations between 1 and 100 milliarcsec (mas) remain mostly unknown due to intrinsic observational limitations. At a typical distance of 2 kpc, this corresponds to projected ph
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