The Kepler space mission provided near-continuous and high-precision photometry of about
207 000 stars, which can be used for asteroseismology. However, for successful seismic …

We have observed and spatially resolved a set of seven A-type stars in the nearby Ursa
Major moving group with the Classic, CLIMB, and PAVO beam combiners on the Center for …

We present chemical composition and fundamental parameters (the effective temperature,
surface gravity, and radius) for four sharp-lined A-type stars γ Gem (HD 41705), o Peg (HD …

Stars of spectral types O and B produce neutron stars (NSs) after supernova explosions.
Most of NSs are strongly magnetized including normal radio pulsars with B∝ 1012 G and …

Context. Intermediate-mass stars are often fast rotators, and hence are centrifugally flattened
and notably affected by gravity darkening. To analyse this kind of stars properly, one must …

We developed a comprehensive model atom of Sc ii–Sc iii. Abundances of scandium for a
sample of eight unevolved A9–B3-type stars with well-determined atmospheric parameters …

We present the spectrum analysis of the hot Am star HR 3383 (A1 Vm). Hubble Space
Telescope STIS and Nordic Optical Telescope SOFIN data are modelled with synthetic …

Aims. We revisit large spectroscopic data sets for field stars from the literature to derive the
upper Li envelope in the high metallicity regime in our Galaxy. Methods. We take advantage …

Inspired by the so appealing example of red giants, where going from a handful of stars to
thousands revealed the structure of the eigenspectrum, we inspected a large homogeneous …

We present accurate element abundance patterns based on the non-local thermodynamic
equilibrium (non-LTE, NLTE) line formation for 14 chemical elements from He to Nd for a …