2756 20160701171710.0 10.1051/eas/1364053 DOI ASTROimport-913 Bakis, V. 2013 V2107 Cyg: A Young Cyg OB1 Member Binary System With A ß Cep Type Pulsating Component V2107 Cyg is located in the direction of Cyg OB1 stellar association. The eclipsing system consists of an early-B primary and a late-B type secondary component contributing about 6% of the total light. Line profile variability and photometry suggest strongly it is a ß Cep type non-radial pulsator. A signature of the faint secondary component is for the first time identified through spectra disentangling. Hensberge, H. Bilir, S. Bakis, H. Demircan, O. Zejda, M. Mikulášek, Z. EAS Publications Series 64 2013 377-378 http://esoads.eso.org/abs/2013EAS....64..377B published in NONREF