Context. Extremely metal-poor (XMP) galaxies are chemically, and possibly dynamically, primordial objects in the local Universe. Aims. Our objective is to characterize the H
Galaxies come in different shapes, sizes, ages, and compositions. Our study\u27s goal is to audit a ...
International audienceThe advent of 8 m class telescopes has allowed the detailed spectroscopic stud...
International audienceThe investigation of the metal-poor tail in the Galactic bulge provides unique...
Extremely metal-deficient (XMD) galaxies, by definition, have oxygen abundances ≠1/10 solar, and for...
Context. Low-metallicity star-forming dwarf galaxies are prime targets to understand the c...
Abstract. Metallicity is a key parameter that controls many aspects in the formation and evolution o...
We demonstrate a successful strategy for identifying extremely metal-poor galaxies. Our preliminary ...
We summarize the progress in identifying and observational study of extremely metal-deficient (...
We report the discovery of eight new extremely metal poor galaxies [XMPGs; 12+log(O/H) lt;7.65...
International audienceCosmic history has witnessed the lives and deaths of multiple generations of m...
The most metal-poor stars provide important constraints on a number of problems, including the model...
Context. The extremely metal-poor stars are the direct descendants of the first generation stars. Th...
International audienceContext: Individual stars in dwarf spheroidal galaxies around the Milky Way Ga...
International audienceContext. Unevolved metal-poor stars bore witness to the early evolution of the...
paper) stars are stars formed in the early universe in terms of chemical evolution. They are formed ...
Galaxies come in different shapes, sizes, ages, and compositions. Our study\u27s goal is to audit a ...
International audienceThe advent of 8 m class telescopes has allowed the detailed spectroscopic stud...
International audienceThe investigation of the metal-poor tail in the Galactic bulge provides unique...
Extremely metal-deficient (XMD) galaxies, by definition, have oxygen abundances ≠1/10 solar, and for...
Context. Low-metallicity star-forming dwarf galaxies are prime targets to understand the c...
Abstract. Metallicity is a key parameter that controls many aspects in the formation and evolution o...
We demonstrate a successful strategy for identifying extremely metal-poor galaxies. Our preliminary ...
We summarize the progress in identifying and observational study of extremely metal-deficient (...
We report the discovery of eight new extremely metal poor galaxies [XMPGs; 12+log(O/H) lt;7.65...
International audienceCosmic history has witnessed the lives and deaths of multiple generations of m...
The most metal-poor stars provide important constraints on a number of problems, including the model...
Context. The extremely metal-poor stars are the direct descendants of the first generation stars. Th...
International audienceContext: Individual stars in dwarf spheroidal galaxies around the Milky Way Ga...
International audienceContext. Unevolved metal-poor stars bore witness to the early evolution of the...
paper) stars are stars formed in the early universe in terms of chemical evolution. They are formed ...
Galaxies come in different shapes, sizes, ages, and compositions. Our study\u27s goal is to audit a ...
International audienceThe advent of 8 m class telescopes has allowed the detailed spectroscopic stud...
International audienceThe investigation of the metal-poor tail in the Galactic bulge provides unique...
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