International audienceWe present the non-local thermodynamic equilibrium (NLTE) abundances of up to 10 chemical species in a sample of 59 very metal-poor (VMP, −4 ≤ [Fe/H] ≾−2) stars in seven dwarf spheroidal galaxies (dSphs) and in the Milky Way (MW) halo. Our results are based on high-resolution spectroscopic datasets and homogeneous and accurate atmospheric parameters determined in Paper I. We show that once the NLTE effects are properly taken into account, all massive galaxies in our sample, that is, the MW halo and the classical dSphs Sculptor, Ursa Minor, Sextans, and Fornax, reveal a similar plateau at [α/Fe] ≃ 0.3 for each of the α-process elements: Mg, Ca, and Ti. We put on a firm ground the evidence for a decline in α/Fe with incr...
We have used the Ultraviolet Echelle Spectrograph (UVES) on Kueyen (UT2) of the Very Large Telescope...
Context. We present a large homogeneous set of stellar parameters and abundances across a broad rang...
International audienceWe present detailed chemical abundances for 99 red-giant branch stars in the c...
International audienceWe present the non-local thermodynamic equilibrium (NLTE) abundances of up to ...
We present the non-local thermodynamic equilibrium (NLTE) abundances of up to 10 chemical species in...
International audienceWe present a homogeneous set of accurate atmospheric parameters for a sample o...
We present atmospheric parameters and abundances for chemical elements from carbon to barium in meta...
International audienceABSTRACT We present atmospheric parameters and abundances for chemical element...
International audienceWe present a homogeneous set of accurate atmospheric parameters for a complete...
We present a homogeneous set of accurate atmospheric parameters for a complete sample of very and ex...
Context. Ultra-faint dwarf galaxies recently discovered around the Milky Way (MW) contain extremely ...
International audienceContext. Metal-poor components of dwarf galaxies around the Milky Way could be...
We have used the Ultraviolet Echelle Spectrograph (UVES) on Kueyen (UT2) of the Very Large Telescope...
Context. We present a large homogeneous set of stellar parameters and abundances across a broad rang...
International audienceWe present detailed chemical abundances for 99 red-giant branch stars in the c...
International audienceWe present the non-local thermodynamic equilibrium (NLTE) abundances of up to ...
We present the non-local thermodynamic equilibrium (NLTE) abundances of up to 10 chemical species in...
International audienceWe present a homogeneous set of accurate atmospheric parameters for a sample o...
We present atmospheric parameters and abundances for chemical elements from carbon to barium in meta...
International audienceABSTRACT We present atmospheric parameters and abundances for chemical element...
International audienceWe present a homogeneous set of accurate atmospheric parameters for a complete...
We present a homogeneous set of accurate atmospheric parameters for a complete sample of very and ex...
Context. Ultra-faint dwarf galaxies recently discovered around the Milky Way (MW) contain extremely ...
International audienceContext. Metal-poor components of dwarf galaxies around the Milky Way could be...
We have used the Ultraviolet Echelle Spectrograph (UVES) on Kueyen (UT2) of the Very Large Telescope...
Context. We present a large homogeneous set of stellar parameters and abundances across a broad rang...
International audienceWe present detailed chemical abundances for 99 red-giant branch stars in the c...