322 citations · 3.7k across the 69 of their papers we have counts for
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NLTE carbon abundance determination in selected A- and B-type stars and the interpretation of C\ione\ emission lines
S. A. Alexeeva, T. A. Ryabchikova, L. I. Mashonkina
We constructed a comprehensive model atom for C\ione\ -- C\ii\ using the most up-to-date atomic data available and evaluated the non-local thermodynamic equilibrium (NLTE) line for…
The Gaia-ESO survey: Hydrogen lines in red giants directly trace stellar mass
Maria Bergemann, Aldo Serenelli, Ralph Schoenrich +27
Red giant stars are perhaps the most important type of stars for Galactic and extra-galactic archaeology: they are luminous, occur in all stellar populations, and their surface tem…
A NLTE line formation for neutral and singly-ionised titanium in model atmospheres of the reference A-K stars
T. M. Sitnova, L. I. Mashonkina, T. A. Ryabchikova
We construct a comprehensive model atom for TiI-II using more than 3600 measured and predicted energy levels of TiI and 1800 energy levels of TiII, and quantum mechanical photoioni…
Influence of Inelastic Collisions with Hydrogen Atoms on the Formation of Al I and Si I Lines in Stellar Spectra
Lyudmila Mashonkina, Andrey K. Belyaev, Jianrong Shi
The non-LTE line formation for Al I and Si I was calculated with model atmospheres corresponding to F-G-K type stars of different metallicity. To account for inelastic collisions w…