http://arxiv.org/abs/2211.07529
We present the first evidence on the $\delta$~Sct type pulsations of the primary components of three eclipsing binaries IQ CMa, AW Men and W Vol in the TESS field. A comprehensive investigation of the binary properties is conducted. The light curves of the systems are analysed and the frequency analyses are performed to residual data. The systems are compared to the binaries of the same morphological types, and the primaries are examined in contrast to the $\delta$~Sct type pulsators. The results show that the systems are oscillating eclipsing Algol-type systems.
B. Ulas and C. Ulusoy
Tue, 15 Nov 22
13/103
Comments: Accepted for publication in Monthly Notices of the Royal Astronomical Society, 14 pages, 13 figures