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 …

The angular momentum (AM) evolution of stellar interiors, along with the resulting rotation
rates of stellar remnants, remains poorly understood. Asteroseismic measurements of red …

Stars lose a significant amount of angular momentum between birth and death, implying that
efficient processes transporting it from the core to the surface are active. Space …

We study the fraction of stars in and around the δ Scuti instability strip that are pulsating,
using Gaia DR2 parallaxes to derive precise luminosities. We classify a sample of over 15 …

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 …

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 …

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 …

Thus far, KIC 7760680 is the richest slowly pulsating B star, exhibiting 36 consecutive dipole
(ℓ= 1) gravity (g-) modes. The monotonically decreasing period spacing of the series, in …

The δ Sct stars are a diverse group of intermediate-mass pulsating stars located on and near
the main sequence within the classical instability strip in the Hertzsprung–Russell diagram …