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Findings of a few recent asteroseismic studies of the main-sequence pulsating stars, as performed in Wojciech Dziembowskis group in Warsaw and in Michel Bregers group in Vienna, are briefly presented and discussed. The selected objects are three hybrid pulsators Nu Eridani, 12 Lacertae and Gamma Pegasi, which show both Beta Cephei and SPB type modes, and the Delta Scuti type star 44 Tauri.
The large-scale magnetic fields detected at the surface of about 10% of hot stars extend into the stellar interior, where they may alter the structure. Deep inner regions of stars are only observable using asteroseismology. Here, we investigated the
We analyse time-series observations from the BRITE-Constellation of the well known $beta$ Cephei type star $theta$ Ophiuchi. Seven previously known frequencies were confirmed and nineteen new frequency peaks were detected. In particular, high-order g
Context: Being part of the brightest solar-like stars, and close solar analogues, the 16 Cygni system is of great interest to the scientific community and may provide insight into the past and future evolution of our Sun. It has been observed thoroug
Results of mode identification and seismic modelling of the $beta$ Cep/SBP star 12 Lacertae are presented. Using data on the multi-colour photometry and radial velocity variations, we determine or constrain the mode degree, $ell$, for all pulsational
Asteroseismology is a unique tool that can be used to study the interior of stars and hence deliver unique information for the studiy of stellar physics, stellar evolution, and Galactic archaeology. We aim to develop a simple model of the informati