V2107 Cyg: A Young Cyg OB1 Member Binary System With A Beta Cep Type Pulsating Component

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Authors	BAKIS Volkan HENSBERGE Herman BILIR S. BAKIS Hicran DEMIRCAN Osman ZEJDA Miloslav MIKULÁŠEK Zdeněk
Year of publication	2013
Type	Article in Periodical
Magazine / Source	European Astronomical Society Publications Series
MU Faculty or unit	Faculty of Science
Citation
Doi	https://doi.org/10.1051/eas/1364053
Field	Astronomy and astrophysics
Keywords	eclipsing binary; beta Cephei; stellar pulsation; OB stellar association
Description	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 beta Cep type non-radial pulsator. A signature of the faint secondary component is for the first time identified through spectra disentangling.
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