7347 20250116195608.0 10.1017/pasa.2024.76 DOI SCART-2025-0034 Kahraman Aliçavuş, Filiz On the existence of `Maia variables' 2024 There are different classes of pulsating stars in the H-R diagram. While many of those classes are undisputed, some remain a mystery such as the objects historically called ‘Maia variables’. Whereas the presence of such a class was suggested seven decades ago, no pulsational driving mechanism is known that could excite short-period oscillations in these late B to early A-type stars. Alternative hypotheses that would render the reports of variability of those stars erroneous have been proposed such as incorrect effective temperatures, binarity or rapid rotation, but no certain conclusions have been reached yet. Therefore, the existence of these variables as a homogeneous class of pulsating star is still under discussion. Meanwhile, many new candidates of these variables have been claimed especially by using photometric observations of space telescopes. In this study, we examined 31 objects that are alleged members of this hypothetical group and carried out detailed spectroscopic and photometric analyses to test the proposed hypotheses for their cause of variability. The Teff, log g, v sin i, and chemical abundances of the targets were determined and the TESS photometric data were examined. As a result, we found that most of these targets are located inside the δ Scuti, β Cephei, or SPB star instability strips, a few show evidence for binarity and others for rapid rotation. We give arguments that none of the apparently rapid pulsations in our targets is caused by a star outside any known instability strip. By extrapolation, we argue that most stars proposed as pulsators outside well-established instability domains are misclassified. Hence there is no sufficient evidence justifying the existence of a class of pulsating stars formerly known as the ‘Maia variables’. NO Stars: oscillations Stars: variables: general Techniques: photometric Techniques: spectroscopic Astrophysics Solar and Stellar Astrophysics Handler, Gerald Chowdhury, Sowgata Niemczura, Ewa Jayaraman, Rahul De Cat, Peter Ozuyar, Dogus Aliçavuş, Fahri Publications of the Astronomical Society of Australia 41 2024 e082 peter.decat@ksb-orb.be 3174070 http://publi2-as.oma.be/record/7347/files/KahramanAliçavuş2024_PASA41_e82.pdf 20461 http://publi2-as.oma.be/record/7347/files/KahramanAliçavuş2024_PASA41_e82.gif?subformat=icon icon 23679 http://publi2-as.oma.be/record/7347/files/KahramanAliçavuş2024_PASA41_e82.jpg?subformat=icon-180 icon-180 published in REFERD