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Solar system abundances and condensation temperatures of the halogens fluorine, chlorine, bromine, and iodine
Neon Abundances of B Stars in the Solar Neighborhood
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Rotation and spots in normal A and Am/Fm stars
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Semiclassical perturbation Stark shifts of singly charged argon spectral lines
Rafik Hamdi, Nabil Ben Nessib, Sylvie Sahal-Bréchot and Milan S Dimitrijević Monthly Notices of the Royal Astronomical Society 488(2) 2473 (2019) https://doi.org/10.1093/mnras/stz1835
Photospheric carbon, nitrogen, and oxygen abundances of A-type main-sequence stars
Yoichi Takeda, Satoshi Kawanomoto, Naoko Ohishi, Dong-Il Kang, Byeong-Cheol Lee, Kang-Min Kim and Inwoo Han Publications of the Astronomical Society of Japan 70(5) (2018) https://doi.org/10.1093/pasj/psy091
High-resolution abundance analysis of the metallic-line star HR 7250
A NLTE line formation for neutral and singly ionized calcium in model atmospheres of B-F stars
T M Sitnova, L I Mashonkina and T A Ryabchikova Monthly Notices of the Royal Astronomical Society 477(3) 3343 (2018) https://doi.org/10.1093/mnras/sty810
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A non-local thermodynamical equilibrium line formation for neutral and singly ionized titanium in model atmospheres of reference A–K stars
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NLTE carbon abundance determination in selected A- and B-type stars and the interpretation of C i emission lines
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Relating turbulent pressure and macroturbulence across the HR diagram with a possible link toγDoradus stars
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On the Application of Stark Broadening Data Determined with a Semiclassical Perturbation Approach
Stark parameter measurement of Ar ii UV spectral lines
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Influence of Departures from LTE on Oxygen Abundance Determination in the Atmospheres of A – K stars
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A high-resolution spectropolarimetric survey of Herbig Ae/Be stars – I. Observations and measurements★
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The first planet detected in the WTS: an inflated hot Jupiter in a 3.35 d orbit around a late F star
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Chemical abundances of magnetic and non-magnetic Herbig Ae/Be stars
LOOKING FOR A CONNECTION BETWEEN THE Am PHENOMENON AND HYBRID δ Sct -γ Dor PULSATION: DETERMINATION OF THE FUNDAMENTAL PARAMETERS AND ABUNDANCES OF HD 114839 AND BD +18 4914