An eclipsing double-line spectroscopic binary at the stellar/substellar boundary in the Upper Scorpius OB association
Aims: We aim at constraining evolutionary models at low mass and young ages by identifying interesting transiting system members of the nearest OB association to the Sun, Upper Scorpius (USco), which has been targeted by the Kepler mission. Methods: We produced light curves for M-dwarf members of the USco region that has been surveyed during the
Lodieu, N. et al.
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2015