Gravity darkening and tidally perturbed stellar pulsation in the misaligned exoplanet system WASP-33
arXiv:2203.09618 · doi:10.1051/0004-6361/202243299
Abstract
WASP-33 is one of the few Sct stars with a known planetary companion. By analyzing the stellar oscillations, we search for possible star-planet interactions in the pattern of the pulsation. We made use of the Transit and Light Curve Modeller (TLCM) to solve the light curve from the Transiting Exoplanet Survey Satellite (TESS). We include gravity darkening into our analysis. The stellar oscillation pattern of WASP-33 clearly shows signs of several tidally perturbed modes. We find that there are peaks in the frequency spectrum that are at or near the rd, th and th orbital harmonics ( d). Also, there is a prominent overabundance of pulsational frequencies rightwards of the orbital harmonics, being characteristic of a tidally perturbed stellar pulsation, which is an outcome of star-planet interactions in the misaligned system. There are peaks in both the Sct and Dor ranges of the Fourier spectrum, implying that WASP-33 is a Dor -- Sct hybrid pulsator. The transit light curves are best fitted by a gravity darkened stellar model, and the planet parameters are consistent with earlier determinations.
Accepted in A&A on 12 March 2022, 6 pages, 4 figures
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Cited by in corpus (7)
- The phase curve of the ultra-hot Jupiter WASP-167b as seen by TESS
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- Discovery of a substellar companion in the TESS light curve of the Scuti/ Doradus hybrid pulsator HD 31221
- The coevolution of migrating planets and their pulsating stars through episodic resonance locking
- Stellar pulsations interfering with the transit light curve: configurations with false positive misalignment
- CHEOPS observations confirm nodal precession in the WASP-33 system
- Cleaning WASP-33 b transits from the host star photometric variability: analysis of TESS data from two sectors