Abstract
We present the first evidence for the pulsations of primary components of four eclipsing binary systems. The TESS light
curves of the targets are analyzed, the light and the absolute parameters are derived. Fourier analyses are applied to the
residual data subtracted from the binary models to reveal the pulsational characteristics of the primaries. The components of
the systems are compared to well-known binary systems of the same morphological type. The types of pulsational classes
for the primaries are also discussed. Results show that CPD-30 740 and V1637 Ori are oscillating eclipsing Algol type
binary stars, while HD 97329 and TYC 683-640-1 are found to be detached systems with pulsating primary components. We
conclude that the primary components of the systems are pulsating stars.
curves of the targets are analyzed, the light and the absolute parameters are derived. Fourier analyses are applied to the
residual data subtracted from the binary models to reveal the pulsational characteristics of the primaries. The components of
the systems are compared to well-known binary systems of the same morphological type. The types of pulsational classes
for the primaries are also discussed. Results show that CPD-30 740 and V1637 Ori are oscillating eclipsing Algol type
binary stars, while HD 97329 and TYC 683-640-1 are found to be detached systems with pulsating primary components. We
conclude that the primary components of the systems are pulsating stars.
| Original language | English |
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| Publication status | Published - Feb 28 2022 |