Something borrowed, something blue: The nature of blue metal-poor stars inferred from their colours and chemical abundances
Author:
Publisher
EDP Sciences
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://www.aanda.org/10.1051/0004-6361/201629628/pdf
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1. Non-LTE oxygen line formation in 3D hydrodynamic model stellar atmospheres
2. NLTE determination of the aluminium abundance in a homogeneous sample of extremely metal-poor stars
3. Evolution of the barium abundance in the early Galaxy from a NLTE analysis of the Ba lines in a homogeneous sample of EMP stars
4. EXAMINATION OF THE MASS-DEPENDENT Li DEPLETION HYPOTHESIS BY THE Li ABUNDANCES OF THE VERY METAL-POOR DOUBLE-LINED SPECTROSCOPIC BINARY G166-45
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1. Chemo-Dynamical Abundance Analysis of the Very Metal-Poor Halo Star HE 2315–4240;International Journal of Applied Physics and Mathematics;2024
2. Field blue straggler stars: discovery of white dwarf companions to blue metal-poor stars using UVIT/AstroSat;Monthly Notices of the Royal Astronomical Society;2023-08-07
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