Yearslong time series of high-precision brightness measurements have been assembled for
thousands of stars with telescopes operating in space. Such data have allowed astronomers …

Asteroseismology provides us with a unique opportunity to improve our understanding of
stellar structure and evolution. Recent developments, including the first systematic studies of …

We present the first asteroseismic results for δ Scuti and γ Doradus stars observed in
Sectors 1 and 2 of the TESS mission. We utilize the 2-min cadence TESS data for a sample …

We present Kepler photometry and ground-based spectroscopy of KIC 4544587, a short-
period eccentric eclipsing binary system with self-excited pressure and gravity modes, tidally …

The catalogue contains 199 confirmed cases of binary systems containing at least one
pulsating component of δ Sct type. The sample is divided into subgroups in order to describe …

We have examined the period–luminosity (P–L) relation for δ Scuti stars using Gaia DR2
parallaxes. We included 228 stars from the catalogue of Rodríguez et al., as well as 1124 …

The distances to four galaxies and two globular clusters which are derived with the aid of
period–luminosity and period–color relations of δ Scuti and SX Phe stars are compared to …

Context. Stellar components in binaries are subject to tidal forces which influence
asteroseismic properties. Tidally pertubed pulsations have been reported for different …

We present Kepler satellite photometry of KIC 10661783, a short-period binary star system
which shows total eclipses and multiperiodic δ Scuti pulsations. A frequency analysis of the …

Context. Fast rotation is responsible for important changes in the structure and evolution of
stars and the way we see them. Optical long baseline interferometry now allows for the study …