The seismic study of the Sun and other stars offers a unique window into the interior of these
stars. Thanks to helioseismology, we know the structure of the Sun to admirable precision. In …

THE application of seismology to the study of the solar interior1, 2 (helioseismology) has
advanced almost solely by the prediction and measurement of the Sun's frequencies of free …

Asteroseismology of stars that exhibit solar-like oscillations are enjoying a growing interest
with the wealth of observational results obtained with the CoRoT and Kepler missions. In this …

We present estimates of the amplitudes of intrinsically stable stochastically excited radial
oscillations in stars near the main sequence. The amplitudes are determined by the balance …

We have made velocity observations of the star α Centauri B from two sites, allowing us to
identify 37 oscillation modes with l= 0-3. Fitting to these modes gives the large and small …

Establishing relations between global stellar parameters and asteroseismic quantities can
help improve our understanding of stellar astrophysics and facilitate the interpretation of …

Recent observational evidence for magnetic field direction effects on helioseismic signals in
sunspot penumbrae is suggestive of magnetohydrodynamic (MHD) mode conversion …

We investigate a model for the excitation of high-order oscillations in roAp stars. In this
model we assume that the strong concentration of magnetic field about the magnetic poles is …

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 investigate the influence of the ionization of helium on the low-degree acoustic
oscillation frequencies in model solar-type stars. The signature in the oscillation frequencies …