Massive stars are important metal factories in the Universe. They have short and energetic
lives, and many of them inevitably explode as a supernova and become a neutron star or …

We present a new, publicly available set of Los Alamos OPLIB opacity tables for the
elements hydrogen through zinc. Our tables are computed using the Los Alamos ATOMIC …

Context. The lack of high-precision long-term continuous photometric data for large samples
of stars has impeded the large-scale exploration of pulsational variability in the OB star …

The first systematic study of opacity dependence on atomic number at stellar interior
temperatures is used to evaluate discrepancies between measured and modeled iron …

Massive stars play a major role not only in stellar evolution but also galactic evolution theory.
This is because of their dynamical interaction with binary companions, but also because …

Recent re-determination of stellar atmospheric parameters for a sample of stars observed
during the Kepler mission allowed to enlarge the number of Kepler B-type stars. We present …

Pulsations and binarity are both common features of massive stars. The study of pulsating
massive stars in eclipsing binary systems holds great potential for constraining stellar …

Context. In asteroseismology, the pulsation mode frequencies of a star are the fundamental
data that are compared to theoretical predictions to determine a star's interior physics …

ABSTRACT KIC 8264293 is a fast-rotating B-type pulsator observed by Kepler satellite. Its
photometric variability is mainly due to pulsations in high-order g modes. Besides, we …

Context. Empirical evidence for the involvement of nonradial pulsations (NRPs) in the mass
loss from Be stars ranges from (i) a singular case (μ Cen) of repetitive mass ejections …