Massive heartbeat stars from TESS

Abstract

Context. Heartbeat stars are eccentric binaries that exhibit a characteristic shape of brightness changes close to the periastron passage, primarily caused by a variable tidal distortion of the components. Variable tidal potential can drive tidally excited oscillations (TEOs), which are usually gravity modes. Studies of heartbeat stars and TEOs open up new possibilities for probing the interiors of massive stars. There are only a few massive (masses of components ≳2 M⊙) systems of this type that are known thus far. Aims. Using TESS data from the first 16 sectors, we searched for new massive heartbeat stars and TEOs using a sample of over 300 eccentric spectroscopic binaries. Methods. We analysed 2 min and 30 min cadence TESS data. Then we fitted Kumar’s analytical model to the light curves of stars showing heartbeats and performed a times-series analysis of the residuals searching for TEOs and periodic intrinsic variability. Results. We found 20 massive heartbeat systems, of which 7 exhibit TEOs. The TEOs occur at harmonics of orbital frequencies in the range between 3 and 36, with the median value equal to 9, which is lower than those in known Kepler systems with TEOs. The most massive system in this sample is the quadruple star HD 5980, a member of the Small Magellanic Cloud. With a total mass of ∼150 M⊙ it is the most massive system showing a heartbeat. Six stars in the sample of the new heartbeat stars are eclipsing. A comparison of the parameters derived from fitting Kumar’s model and from light-curve modelling shows that Kumar’s model does not provide reliable parameters. In other words, the orbital parameters can be reliably derived from fitting heartbeat light curves only if the model includes all proximity effects. Finally, intrinsic pulsations of β Cep, SPB, δ Sct, and γ Dor-type were found in nine heartbeat systems. This opens an interesting possibility for studies of pulsation-binarity interaction and the co-existence of forced and self-excited oscillations.

An all-sky sample of intermediate- to high-mass OBA-type eclipsing binaries observed by TESS

“…For this purpose, the approach presented here focuses on eclipsing binary (EB) stars as these present the opportunity to measure model-independent stellar masses and radii. While searches for individual pulsating OB-type EB targets (Southworth et al 2020(Southworth et al , 2021, as well as medium-size samples of interesting targets such as massive heartbeat stars (Kołaczek-Szymański et al 2021), are ongoing, we take a homogeneous systematic large-scale approach. A notable large-scale sample of TESS eclipsing binaries in the Southern Hemisphere that covers a wide range in temperatures using a systematic selection procedure has been compiled by Justesen & Albrecht (2021).…”

Asteroseismology of Close Binary Stars: Tides and Mass Transfer

“…We compile a list of 22 heartbeat binaries with TEOs: OB-type: HD 177863 (Willems and Aerts, 2002); ι Ori (Pablo et al, 2017); MACHO80.7443.1718 (Jayasinghe et al, 2019); QX Car and V1294 Sco (Kołaczek-Szymański et al, 2020); two possible candidates: η Car (Richardson et al, 2018); R81 (Tubbesing et al, 2002).…”

“…A-F-type: HD209295 (Handler et al, 2002); KOI-54 (Welsh et al, 2011); KIC 3230227 (Guo et al, 2017a); KIC 4142768 ; KIC 9016693, KIC 8719324 and KIC 4248941, KIC 5034333 (Guo et al, 2020); KIC 11494130 and KIC 5790807 (Cheng et al, 2020), KIC 4544587 (Hambleton et al, 2013); KIC 3749404 (Hambleton et al, 2016), KIC 8164262 (Fuller et al, 2017;Hambleton et al, 2018); p Vel, θ 1 Cru, η 1 UMa, HD158013 and 14 Peg (Kołaczek-Szymański et al, 2020).…”

Space-Based Photometry of Binary Stars: From Voyager to TESS

“…Kołaczek-Szyma ński et al [280] searched for high-mass heartbeat stars in data from TESS sectors 1-16. They found 20 objects, of which seven show tidally-excited oscillations.…”