activity
19982024
most citedThe chemical abundance analysis of normal early A- and late B-type stars

81 citations · 1.4k across the 56 of their papers we have counts for

collaborators

56 papers

astro-ph.SR2024

Are the surface abundance structures stable in rapidly rotating Ap star 56 Ari?

I. Potravnov, N. Piskunov, T. Ryabchikova

The surface magnetic and abundance inhomogeneities in chemically peculiar Ap/Bp stars are coupled and responsible for their rotationally modulated variability. Within the framework…

astro-ph.SR2023★ 5 cited

Doppler imaging of a southern ApSi star HD 152564

I. Potravnov, T. Ryabchikova, N. Piskunov +2

We present the results of the spectroscopic study of a chemically peculiar star HD 152564. Using medium-resolution () observations obtained with the HRS spectrograph mount…

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…

physics.atom-ph2023★ 1 cited

The Spectrum and Energy Levels of the Low-lying Configurations of Nd III

Milan Ding, Juliet C. Pickering, Alexander N. Ryabtsev +2

Emission spectra of neodymium (Nd, Z=60) were recorded using Penning and hollow cathode discharge lamps in the region 11500-54000 cm (8695-1852 Å) by Fourier transform spect…

astro-ph.SR2023★ 5 cited

BD+30549: young helium-weak silicon star in NGC 1333 star-forming region

I. Potravnov, L. Mashonkina, T. Ryabchikova

We present results of the spectroscopic study of the chemically peculiar star BD+30549 which is bona-fide member of young NGC 1333 star forming region. We found that the st…

astro-ph.SR2022★ 8 cited

Using Molecular Lines to Determine Carbon and Nitrogen Abundances in the Atmospheres of Cool Stars

T. Ryabchikova, N. Piskunov, Y. Pakhomov

Simultaneous analysis of the C_2 and CN molecular bands in the 5100-5200 and 7930-8100A spectral regions is a promising alternative for the accurate determination of the carbon (C)…