We review the application of the one-dimensional Mixing Length Theory (MLT) model of
convection in stellar interiors and low-mass stellar evolution. We summarize the history of …

Rotation matters for the life of a star. It causes a multitude of dynamical phenomena in the
stellar interior during a star's evolution, and its effects accumulate until the star dies. All stars …

Context. Magnetic fields affect stars at all evolutionary stages. While surface fields have
been measured for stars across the Hertzsprung–Russell (HR) diagram, internal magnetic …

Context. Tens of thousands of red giant stars in the Kepler data exhibit solar-like oscillations.
The mixed-mode characteristics of their oscillations enable us to study the internal physics …

Strong magnetic fields are expected to significantly modify the pulsation frequencies of
waves propagating in the cores of red giants or in the radiative envelopes of intermediate …

Despite major progress in our understanding of massive stars, concerning discrepancies still
remain between observations and theory. Most notable are the numerous stars observed …

Products of stellar mergers are predicted to be common in stellar populations and can
potentially explain stars with peculiar properties. When the merger occurs after the initially …

Asteroseismology provides a new avenue for accurately measuring the masses of evolved
globular cluster (GC) stars. We present the first detections of solar-like oscillations in 47 red …

Blue large-amplitude pulsators (BLAPs) are a newly discovered type of variable star. Their
typical pulsation periods are on the order of a few tens of minutes, with relatively large …

We present a flow-based generative approach to emulate grids of stellar evolutionary
models. By interpreting the input parameters and output properties of these models as …