activity
20062024
most citedNLTE determination of the aluminium abundance in a homogeneous sample of extremely metal-poor stars

145 citations · 2k across the 48 of their papers we have counts for

collaborators

48 papers

astro-ph.SR2024

Lithium Cepheid V708 Car with an unusual chemical composition

V. V. Kovtyukh, S. M. Andrievsky, K. Werner +2

The purpose of this work is to spectroscopically analyse the classical Cepheid V708 Car. A preliminary check of the spectrum of V708 Car showed that this is a lithium-rich supergia…

astro-ph.SR2023

Non-LTE abundance analysis of A-B stars with low rotational velocities. II. Do A-B stars with normal abundances exist?

A. M. Romanovskaya, T. A. Ryabchikova, Yu. V. Pakhomov +2

We present chemical composition and fundamental parameters (the effective temperature, surface gravity and radius) for four sharp-lined A-type stars Gem (HD 41705), o Peg (HD 2…

astro-ph.SR2023★ 1 cited

Abundance of radioactive technetium in Przybylski's star revisited

S. M. Andrievsky, S. A. Korotin, K. Werner

We have searched for lines of the radioactive element technetium (Tc) in the spectrum of Przybylski's star (HD101065). The nuclei of this chemical element are formed in the slow pr…

astro-ph.SR2023★ 1 cited

An enigma of Przybylski's star: is there promethium on its surface?

Sergei M. Andrievsky, Sergey A. Korotin, Klaus Werner +1

We carried out a new attempt to check for the presence promethium lines in the spectrum of HD101065 (Przybylski's star). The neutron capture element promethium does not have stable…

astro-ph.SR2021★ 5 cited

NLTE CNO abundances in a sample of nine field RR lyr type stars

Sergei M. Andrievsky, Sergey A. Korotin, Valery V. Kovtyukh +2

For the first time, a direct NLTE analysis of carbon and nitrogen lines in the spectra of nine RR Lyrae stars was carried out. We have determined the abundances of these elements t…

astro-ph.SR2021★ 4 cited

Rubidium abundances in solar metallicity stars

C. Abia, P. de Laverny, S. Korotin +3

A Rb deficiency by a factor two with respect to the Sun has been found in M dwarfs of solar metallicity. This deficiency is difficult to understand from both the observational and…