The early 21st century is witnessing a breakthrough in the study of the thermal radiation of
neutron stars. Observations with modern space telescopes have provided a wealth of …

Magnetic storms on stars manifest as remarkable, randomly occurring changes of the
luminosity over durations that are tiny in comparison to the normal evolution of stars. These …

We present improved calculations for the Stark broadening of hydrogen lines in dense
plasmas typical of white dwarf atmospheres. Our new model is based on the unified theory …

New tables of Stark broadened hydrogen Lyman, Balmer and Paschen lines are presented
for a wide range of plasma conditions, allowing the complete spectrum of these series to be …

Redshifted components of chromospheric emission lines in the hard X-ray impulsive phase
of solar flares have recently been studied through their 30 s evolution with the high …

Details of a theory of self-broadening of hydrogen lines are presented. The main features of
the new theory are that the dispersive-inductive components of the interaction (van der …

The heating mechanism at high densities during M-dwarf flares is poorly understood.
Spectra of M-dwarf flares in the optical and near-ultraviolet wavelength regimes have …

Spectral line-shape models are an important part of understanding high-energy-density
(HED) plasmas. Models are needed for calculating opacity of materials and can serve as …

The low-frequency electric microfield distribution in a Coulomb plasma is calculated for
various plasma parameters, from weak to strong Coulomb coupling and from zero to strong …

Stark broadening of hydrogen Lyman and Balmer in the conditions of stellar envel ADS Classic
is now deprecated. It will be completely retired in October 2019. This page will automatically …