New ultra metal-poor stars from SDSS: follow-up GTC medium-resolution spectroscopy
Context. The first generation of stars formed in the Galaxy left behind the chemical signatures of their nucleosynthesis in the interstellar medium, visible today in the atmospheres of low-mass stars that formed afterwards. Sampling the chemistry of those low-mass provides insight into the first stars. Aims: We aim to increase the samples of stars
Aguado, D. S. et al.
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2017