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 has grown from its beginnings three decades ago to a mature field
teeming with discoveries and applications. This phenomenal growth has been enabled by …

Context. Gamma Doradus stars (hereafter γ Dor stars) are known to exhibit gravity-and/or
gravito-intertial modes that probe the inner stellar region near the convective core boundary …

Context. The Kepler spacecraft is providing time series of photometric data with
micromagnitude precision for hundreds of AF type stars. Aims. We present a first general …

We report our survey of γ Dor stars from the 4-yr Kepler mission. These stars pulsate mainly
in g modes and r modes, showing period-spacing patterns in the amplitude spectra. The …

Asteroseismology involves probing the interiors of stars and quantifying their global
properties, such as radius and age, through observations of normal modes of oscillation …

Context. The Gaia mission has delivered hundreds of thousands of variable star light curves
in multiple wavelengths. Recent work demonstrates that these light curves can be used to …

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 apply here the Time Dependent Convection (TDC) treatment presented in our earlier
paper in this series to the study of δ Sct and γ Dor pulsating stars. Stabilization of the δ Sct p …

Observations of the pulsations of stars can be used to infer their interior structure and test
theoretical models. The main-sequence γ Doradus (Dor) and δ Scuti (Sct) stars with masses …