The rapidly increasing number of delta Scuti stars with regular patterns among their
pulsation frequencies necessitates modelling tools to better understand the observations …

The bright star λ Ser hosts a hot Neptune with a minimum mass of 13.6 M⊕ and a 15.5 day
orbit. It also appears to be a solar analog, with a mean rotation period of 25.8 days and …

Although stellar radii from asteroseismic scaling relations agree at the per cent level with
independent estimates for main sequence and most first-ascent red giant branch (RGB) …

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 …

Abstract Very-metal-poor stars ([Fe/H]<− 2) are important laboratories for testing stellar
models and reconstructing the formation history of our galaxy. Asteroseismology is a …

Asteroseismic modeling is a powerful way to derive stellar properties. However, the derived
quantities are limited by built-in assumptions used in stellar models. This work presents a …

This paper reports the estimated stellar parameters of 1153 Kepler red giant branch stars
determined with asteroseismic modeling. We use radial-mode oscillation frequencies …

Nearly all cool, evolved stars are solar-like oscillators, and fundamental stellar properties
can be inferred from these oscillations with asteroseismology. Scaling relations are …

The importance of νmax (the frequency of maximum oscillation power) for asteroseismology
has been demonstrated widely in the previous decade, especially for red giants. With the …

Asteroseismology is our only means of measuring the rotations of stars in their interiors,
rather than at their surfaces. Some techniques for measurements of this kind—" rotational …