Aims. We investigate the formation of neutral and singly ionized scandium lines in the solar photospheres. The research is aimed at derive solar $\log gf\varepsilon_{\odot}$(Sc) values for scandium lines, which will later be used in differential abundance analyses of metal-poor stars. Methods. Extensive statistical equilibrium calculations were carried out for a model atom, which comprises 92 terms for Sc
We redetermine the abundances of all iron group nuclei in the Sun, based on neutral and si...
Distribution study with Sc46 as tracer and ammonium ferric alum as host Iattice at 4° shows that the...
Our ability to model the shapes and strengths of iron lines in the solar spectrum is a critical test...
Aims. We investigate the formation of neutral and singly ionized scandium lines in the solar photosp...
We investigate the formation of neutral and singly ionized scandium lines in the solar photospheres....
The lifetimes of 17 even-parity levels (3d5s, 3d4d, 3d6s, and 4p$^2$) in the region 57743-77837 cm$^...
The lifetimes of 17 even-parity levels (3d5s, 3d4d, 3d6s and 4p2) in the region 57 743–77 837 cm−1 o...
A new model atom of Sc II was constructed using the most up-to-date atomic data. For the testing pur...
Aims. The statistical equilibrium of neutral and ionized silicon in the atmospheres of metal-poor st...
Aims. The statistical equilibrium of neutral and ionised silicon in the solar photosphere is investi...
We redetermine the abundances of all iron group nuclei in the Sun, based on neutral and singly-ionis...
Context. Spectroscopic data for scandium is sparse, while an extensive set is needed to in...
We redetermine the abundances of all iron group nuclei in the Sun, based on neutral and singly-ionis...
International audienceAtomic symbol: Sc Atomic number: 21 Atomic weight: 44.95591 Isotopes and abund...
New branching fraction (BF) measurements for lines of Sc i and Sc ii from 24 Fourier transform spect...
We redetermine the abundances of all iron group nuclei in the Sun, based on neutral and si...
Distribution study with Sc46 as tracer and ammonium ferric alum as host Iattice at 4° shows that the...
Our ability to model the shapes and strengths of iron lines in the solar spectrum is a critical test...
Aims. We investigate the formation of neutral and singly ionized scandium lines in the solar photosp...
We investigate the formation of neutral and singly ionized scandium lines in the solar photospheres....
The lifetimes of 17 even-parity levels (3d5s, 3d4d, 3d6s, and 4p$^2$) in the region 57743-77837 cm$^...
The lifetimes of 17 even-parity levels (3d5s, 3d4d, 3d6s and 4p2) in the region 57 743–77 837 cm−1 o...
A new model atom of Sc II was constructed using the most up-to-date atomic data. For the testing pur...
Aims. The statistical equilibrium of neutral and ionized silicon in the atmospheres of metal-poor st...
Aims. The statistical equilibrium of neutral and ionised silicon in the solar photosphere is investi...
We redetermine the abundances of all iron group nuclei in the Sun, based on neutral and singly-ionis...
Context. Spectroscopic data for scandium is sparse, while an extensive set is needed to in...
We redetermine the abundances of all iron group nuclei in the Sun, based on neutral and singly-ionis...
International audienceAtomic symbol: Sc Atomic number: 21 Atomic weight: 44.95591 Isotopes and abund...
New branching fraction (BF) measurements for lines of Sc i and Sc ii from 24 Fourier transform spect...
We redetermine the abundances of all iron group nuclei in the Sun, based on neutral and si...
Distribution study with Sc46 as tracer and ammonium ferric alum as host Iattice at 4° shows that the...
Our ability to model the shapes and strengths of iron lines in the solar spectrum is a critical test...