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Published in 2018 at "Astronomy and Astrophysics"
DOI: 10.1051/0004-6361/201732320
Abstract: Context. Extremely metal-poor (EMP) stars provide us with indirect information on the first generations of massive stars. The TOPoS survey has been designed to increase the census of these stars and to provide a chemical…
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Keywords:
poor stars;
metal poor;
sdss;
extremely metal ... See more keywords
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Published in 2020 at "Astronomy and Astrophysics"
DOI: 10.1051/0004-6361/202039101
Abstract: Abundances of beryllium in metal-poor stars scale linearly with metallicity down to [Fe/H] ~ -3.0. In the stars where Be has been detected at this extremely metal-poor regime, an increased abundance scatter has been previously…
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Keywords:
poor stars;
metal poor;
abundances extremely;
inhomogeneity early ... See more keywords
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Published in 2018 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/sty1920
Abstract: This study in based on observations collected at the European Southern Observatory. We are very grateful to our referee for providing constructive comments and help in improving the manuscript. This work has been partially funded…
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Keywords:
metal poor;
extremely metal;
poor galaxy;
extended 4686 ... See more keywords
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1
Published in 2018 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/sty2783
Abstract: Extremely metal poor (EMP) stars in the Milky Way inherited the chemical composition of the gas out of which they formed. They therefore carry the chemical fingerprint of the first stars in their spectral lines.…
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Keywords:
metal poor;
extremely metal;
first stars;
fingerprint first ... See more keywords
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1
Published in 2022 at "Physical review letters"
DOI: 10.1103/physrevlett.130.131001
Abstract: The recent measurement of helium-4 from the near-infrared spectroscopy of extremely metal-poor galaxies by the Subaru Survey may point to a new puzzle in the early Universe. We exploit this new helium measurement together with…
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Keywords:
poor galaxies;
nonzero lepton;
metal poor;
extremely metal ... See more keywords