To better understand the hot chemically peculiar group of HgMn stars, we have considered a
compilation of a large number of recently published data obtained for these stars from …

Using high-resolution, high-signal-to-noise ratio archival UVES (Ultraviolet-Visual Echelle
Spectrograph) spectra, we have performed a detailed spectroscopic analysis of four …

The abundances of 14 elements in the atmospheres of 20 sharp-lined Hg–Mn stars were
derived from published equivalent widths and microdensitometer tracings of high-resolution …

Recent results obtained by various authors on the properties of HgMn stars are reviewed.
Substantial progress has been achieved in the study of abundances and isotopic anomalies …

In this paper, we present a new catalogue of chemically peculiar (CP) stars obtained by
compiling publications in which abundances of metals are provided. Our catalogue includes …

We report on H-band spectra of chemically peculiar Mercury–Manganese (HgMn) stars
obtained via the SDSS/APOGEE survey. As opposed to other varieties of chemically peculiar …

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 …

Optical region spectra of 31 HgMn stars have been studied for the abundance and isotope
mixture of mercury. In the course of the investigation the lines λ4358 and λ λ3984, 6149 …

Theoretical models addressing the origin of peculiarities in the spectra of HgMn stars have
not been sufficiently constrained so far by the available abundance data. Previous studies of …

In this paper, we present a multi-instrument analysis of the mercury-manganese star HD
49606. New spectroscopic observations have been obtained by us with Catania …