The convective envelopes of solar-type stars and the convective cores of intermediate-and
high-mass stars share boundaries with stable radiative zones. Through a host of processes …

Asteroseismology probes the internal structures of stars by using their natural pulsation
frequencies. It relies on identifying sequences of pulsation modes that can be compared with …

We present the results of a systematic search for new rapidly oscillating Ap (roAp) stars
using the 2-min cadence data collected by the Transiting Exoplanet Survey Satellite (TESS) …

We investigate the relationship between the asteroseismic indices and the physical
quantities of 438 δ Scuti (DSCT) stars observed by the Transiting Exoplanet Survey Satellite …

Since the end of 2018, the Transiting Exoplanet Survey Satellite (TESS) has provided stellar
photometry to the astronomical community. We have used TESS data to study rotational …

Abstract δ Scuti variables are stars which exhibit periodic changes in their luminosity
through radial and nonradial pulsations. Internally, these stars have relatively small …

Since the end of 2018, the Transiting Exoplanet Survey Satellite (TESS) provides high-
quality space data on stellar photometry to the astronomical community. We present the …

With the upcoming plethora of astronomical time-domain datasets and surveys, anomaly
detection as a way to discover new types of variable stars and transients has inspired a new …

δ Scuti (δ Sct) variables are stars exhibiting variations in their luminosity from low radial
order pressure modes and mixed modes, and these pulsations typically last anywhere from …

We investigate the relationship between the asteroseismic indices and the physical
quantities of 438 Scuti (DSCT) stars observed by the Transiting Exoplanet Survey Satellite …