Discovery of β Cep pulsations in the eclipsing binary V453 Cygni. (18th May 2020)

• Record Type: Journal Article
• Authors: Southworth, John; Bowman, D M; Tkachenko, A; Pavlovski, K
• Is Part Of: Monthly notices of the Royal Astronomical Society. Volume 497:Number 1(2020)
• Page Start: L19
• Page End: L23
• Publication Date: 2020-05-18
• Subjects: binaries: eclipsing -- stars: fundamental parameters -- stars: oscillations; Astronomy -- Research -- Periodicals; Periodicals; 520.5
• DOI: 10.1093/mnrasl/slaa091
• Languages: English
• ISSNs: 1745-3933

Abstract

ABSTRACT: V453 Cyg is an eclipsing binary containing 14 and 11 $\, {\rm M}_\odot$ stars in an eccentric short-period orbit. We have discovered β Cep-type pulsations in this system using Transiting Exoplanet Survey Satellite data. We identify seven significant pulsation frequencies, between 2.37 and 10.51 d −1, in the primary star. These include six frequencies that are separated by yet significantly offset from harmonics of the orbital frequency, indicating they are tidally perturbed modes. We have determined the physical properties of the system to high precision: V453 Cyg A is the first β Cep pulsator with a precise mass measurement. The system is a vital tracer of the physical processes that govern the evolution of massive single and binary stars.