We present detailed chemical abundances for 99 red-giant branch stars in the centre of the Sculptor dwarf spheroidal galaxy, which have been obtained from high-resolution VLT/FLAMES spectroscopy. The abundances of Li, Na, alpha-elements (O, Mg, Si, Ca Ti), iron-peak elements (Sc, Cr, Fe, Co, Ni, Zn), and r- and s-process elements (Ba, La, Nd, Eu) were all derived using stellar atmosphere models and semi-automated analysis techniques. The iron abundances populate the whole metallicity distribution of the galaxy with the exception of the very low metallicity tail, -2.3 -2.3 is extremely low, and compatible with observational errors. Combined with the small scatter in the age-elemental abundances relation, this calls for an efficient mixing o...
In Galactic halo stars, sulphur has been shown to behave like other α-elements, but until now, no co...
Context. The ages of individual red giant branch stars can range from 1 Gyr old to the age of the Un...
We have used the Ultraviolet Echelle Spectrograph (UVES) on Kueyen (UT2) of the Very Large Telescope...
We present detailed chemical abundances for 99 red-giant branch stars in the centre of the Sculptor ...
We present detailed chemical abundances for 99 red-giant branch stars in the centre of the Sculptor ...
For the first time we show the detailed, late-stage, chemical evolution history of a small nearby dw...
We present the high-resolution spectroscopic study of five -3.9 ≤ [Fe/H] ≤ -2.5 stars in the Local G...
For the first time we show the detailed, late-stage, chemical evolution history of a small nearby dw...
We present measurements of Fe, Mg, Si, Ca, and Ti abundances for 388 radial velocity member stars in...
VizieR online Data Catalogue associated with article published in journal Astronomy & Astrophysi...
In Galactic halo stars, sulphur has been shown to behave like other α-elements, but until now, no co...
The Sculptor dwarf spheroidal galaxy is a Milky Way satellite with predominantly old stellar populat...
In Galactic halo stars, sulphur has been shown to behave like other α-elements, but until now, no co...
Context. The ages of individual red giant branch stars can range from 1 Gyr old to the age of the Un...
We have used the Ultraviolet Echelle Spectrograph (UVES) on Kueyen (UT2) of the Very Large Telescope...
We present detailed chemical abundances for 99 red-giant branch stars in the centre of the Sculptor ...
We present detailed chemical abundances for 99 red-giant branch stars in the centre of the Sculptor ...
For the first time we show the detailed, late-stage, chemical evolution history of a small nearby dw...
We present the high-resolution spectroscopic study of five -3.9 ≤ [Fe/H] ≤ -2.5 stars in the Local G...
For the first time we show the detailed, late-stage, chemical evolution history of a small nearby dw...
We present measurements of Fe, Mg, Si, Ca, and Ti abundances for 388 radial velocity member stars in...
VizieR online Data Catalogue associated with article published in journal Astronomy & Astrophysi...
In Galactic halo stars, sulphur has been shown to behave like other α-elements, but until now, no co...
The Sculptor dwarf spheroidal galaxy is a Milky Way satellite with predominantly old stellar populat...
In Galactic halo stars, sulphur has been shown to behave like other α-elements, but until now, no co...
Context. The ages of individual red giant branch stars can range from 1 Gyr old to the age of the Un...
We have used the Ultraviolet Echelle Spectrograph (UVES) on Kueyen (UT2) of the Very Large Telescope...