Analysis of Photometric Variability in B-type Stars Observed by the TESS Space Mission
Stellar variability, B-type stars, TESS, photometry
Massive stars are essential for the evolution and chemical enrichment of the universe; however, their structure and evolution remain poorly understood. This work presents a detailed analysis of photometric variability in B-type stars observed by the TESS space mission, in order to expand the number of stars with known rotation periods. The analysis covers 373 B-type stars, observed in 2-minute cadences by the TESS space mission. Three integrated temporal analysis techniques were employed: FFT and Lomb-Scargle periodograms, and wavelet transform, to characterize the variability signatures in the light curves. The classification revealed different types of variability, including 14 new B-type stars with rotational modulation in the TESS data, and 16 previously studied targets had their periods confirmed based on the literature. Among the remaining stars, pulsation signatures, binary systems, and candidates for hot subdwarfs were also identified. It was observed that a significant fraction of the sample exhibits noisy or ambiguous signals, possibly due to observational limitations or complex physical phenomena. The results obtained contribute to the understanding of stellar variability and highlight the importance of combining different analytical methods for identifying patterns in stellar photometry.