Tidally Trapped Two-pole Pulsations Discovered in a Close Binary with a Massive $\beta$ Cephei Star

TL;DR

This paper reports the first detection of tidally trapped two-pole pulsations in a massive $eta$ Cephei star within a close binary system, expanding the class of tidally tilted pulsators and providing new insights into stellar interior and tidal interactions.

Contribution

It is the first to identify tidally trapped pulsations in a $eta$ Cephei star, demonstrating a new class of oscillators influenced by strong tidal forces in massive binaries.

Findings

Discovery of tidally trapped pulsations in HD~329379

Pulsation amplitude modulated with orbital frequency

Pulsations concentrated near tidal poles

Abstract

Tidally tilted pulsators (TTPs), whose pulsation axis aligns with the binary's semi-major axis, represent a newly established class of oscillators in binary systems. While all previously known TTPs are either $\delta$ Scuti or subdwarf B-type stars, their existence has remained unidentified in more massive $\beta$ Cephei variables. Here, we report the discovery of tidally trapped pulsations in the massive ellipsoidal variable HD~329379, based on photometry from the Transiting Exoplanet Survey Satellite (TESS). Our analysis reveals a $\beta$ Cephei pulsator in a 2.25-day orbit whose pulsation mode amplitude is strongly modulated with the orbital frequency. Based on our analysis, we concluded that this modulation can be explained by pulsations with significantly larger amplitude near the star's two tidal poles (apsides). We interpret this as a tidally distorted quadrupole pulsation chariacteristiced by trapped two-pole pulsations, with a pulsation axis aligned with the tidal axis. This represents the first identification of such a pulsation mode in a $\beta$ Cephei star, which differs from single-sided pulsations observed in previous works, marking a rare and important discovery. Our work extends the family of TTPs beyond $\delta$ Scuti and subdwarf B-type stars to include more massive $\beta$ Cephei variables. In particular, the two-pole pulsator HD~329379 stands out as the prototype of a new class of TTPs in massive stars. These results not only provide a new insight to probe the interior structure and evolutionary state for massive stars but also offer a unique opportunity to study the interaction between pulsations and strong tidal distortions.