HD 32239: An Algol type eclipsing binary with a γ Doradus type component

HD 32239 is an Algol-type eclipsing binary with one of the components showing γ Doradus type pulsation. In this study by using the Transiting Exoplanet Survey Satellite (TESS) observations of the HD 32239 system published in Sectors 5 and 32, we obtained the minima times of the eclipsing system and calculated the new light elements by using the (O−C) technique, the out of eclipse variation related to the pulsation was analysed in the frequency domain and g-mode pulsations were detected at frequencies of 1.24–2.83 d−1. After removing the pulsational variation from the light curve we obtained the physical and geometrical parameters of the components by using the well known Wilson–Devinney code.