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Laboratory confirmation and improved accuracy of 4f and 5d energy levels of Fe ii previously identified from stellar spectra
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The Behavior of HgMn Stars in the Far-UV—Paper 7: HR 6000
The NLTE Analyses of Carbon Emission Lines in the Atmospheres of O- and B-type Stars
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NLTE spectroscopic analysis of the3He anomaly in subluminous B-type stars
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Weak metallic emission lines in early B-type stars
NLTE carbon abundance determination in selected A- and B-type stars and the interpretation of C i emission lines
S. A. Alexeeva, T. A. Ryabchikova and L. I. Mashonkina Monthly Notices of the Royal Astronomical Society 462(1) 1123 (2016) https://doi.org/10.1093/mnras/stw1635
Spectroscopic study of the HgMn star HD 49606: the quest for binarity, abundance stratifications and magnetic field
G. Catanzaro, M. Giarrusso, F. Leone, et al. Monthly Notices of the Royal Astronomical Society 460(2) 1999 (2016) https://doi.org/10.1093/mnras/stw923
Abundance analysis, spectral variability, and search for the presence of a magnetic field in the typical PGa star HD 19400
S. Hubrig, F. Castelli, J. F. González, et al. Monthly Notices of the Royal Astronomical Society 442(4) 3604 (2014) https://doi.org/10.1093/mnras/stu1122
HD 161701, a chemically peculiar binary with a HgMn primary and an Ap secondary
Determination of Atmospheric Parameters of B-, A-, F- and G-Type Stars
Robert L. Kurucz GeoPlanet: Earth and Planetary Sciences, Determination of Atmospheric Parameters of B-, A-, F- and G-Type Stars 63 (2014) https://doi.org/10.1007/978-3-319-06956-2_6
Wavelengths and oscillator strengths of Xe II from the UVES spectra of four HgMn stars
Including all the lines1This article is part of a Special Issue on the 10th International Colloquium on Atomic Spectra and Oscillator Strengths for Astrophysical and Laboratory Plasmas.