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B. Bale

4 papers hereh-index 12 citations5 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author2
  • middle author1
  • last author1

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR4

identity via Semantic Scholar / OpenAlex

activity
20232026
collaborators

4 papers

astro-ph.SR2026

The non-LTE abundances of magnesium and yttrium and asteroseismic ages for the chemical clock calibration

Š. Mikolaitis, G. Tautvaišienė, E. Pakštienė +11

Building on our previous study, which demonstrated the importance of accounting for departures from local thermodynamic equilibrium (LTE) in elemental-abundance determinations and…

astro-ph.SR2025

Chromospherically active stars: Lithium and CNO abundances in northern RS CVn stars

B. Bale, G. Tautvaisiene, R. Minkeviciute +4

Aims: We carried out a detailed investigation of Lithium and CNO abundances, including carbon isotope ratios, in RS CVn stars to assess the role of magnetic activity in the mixing…

astro-ph.SR2025

Chromospherically active stars: Chemical composition of photospheres in 20 RS CVn stars

B. Bale, G. Tautvaisiene, R. Minkeviciute +4

Context. Various element transport processes modify the photospheric chemical composition of low-mass stars during their evolution. The most prominent one is the first dredge-up th…

astro-ph.SR2023

12C/13C of Kepler giant stars: the missing piece of the mixing puzzle

N. Lagarde, R. Minkeviciute, A. Drazdauskas +6

Despite a rich observational background, few spectroscopic studies have dealt with the measurement of the carbon isotopic ratio in giant stars. However, it is a key element in unde…

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