activity
20132023
most citedThe formation of the Milky Way halo and its dwarf satellites; a NLTE-1D abundance analysis. II. Early chemical enrichment

76 citations · 192 across the 10 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

14 papers · 1 filter

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

1D non-LTE corrections for chemical abundance analyses of very metal-poor stars

L. Mashonkina, Yu. Pakhomov, T. Sitnova +3

Detailed chemical abundances of very metal-poor (VMP, [Fe/H] < -2) stars are important for better understanding the First Stars, early star formation and chemical enrichment of gal…

astro-ph.SR202119 cited

The Pristine survey XIV: chemical analysis of two ultra-metal-poor stars

C. Lardo, L. Mashonkina, P. Jablonka +15

Elemental abundances of the most metal-poor stars reflect the conditions in the early Galaxy and the properties of the first stars. We present a spectroscopic follow-up of two ultr…

astro-ph.SR2020

Chemical diversity among A-B stars with low rotational velocities: non-LTE abundance analysis

L. Mashonkina, T. Ryabchikova, S. Alexeeva +2

We present accurate element abundance patterns based on the non-local thermodynamic equilibrium (non-LTE, NLTE) line formation for 14 chemical elements from He to Nd for a sample o…

astro-ph.SR2020

Mono-enriched stars and Galactic chemical evolution -- Possible biases in observations and theory

Camilla Juul Hansen, Andreas Koch, Lyudmila Mashonkina +9

A long sought after goal using chemical abundance patterns derived from metal-poor stars is to understand the Galactic chemical evolution (GCE) and to pin down the nature of the fi…

astro-ph.SR202020 cited

Influence of Collisions with Hydrogen on Titanium Abundance Determinations in Cool Stars

T. M. Sitnova, S. A. Yakovleva, A. K. Belyaev +1

We performed the non-local thermodynamic equilibrium (non-LTE) calculations for Ti I-II with the updated model atom that includes quantum-mechanical rate coefficients for inelastic…