We present detailed elemental abundances of 12 subgiants in the open cluster IC 4756 including Na, Al, Mg, Si, Ca, Ti, Cr, Ni, Fe, Zn and Ba. We measure the cluster to have [Fe/H] = -0.01 ± 0.10. Most of the measured star-to-star [X/H] abundance variati
A detailed abundance analysis of 2 giants of the metal-rich bulge globular cluster NGC6553 was carri...
Recent theoretical yields and chemical evolution models demonstrate that intermediate-mass AGB stars...
We present detailed chemical abundance measurements for 45 globular clusters (GCs) associated with g...
International audienceAims: We present the abundance measurements of several elements (Fe, Ca, Na, N...
We present a detailed chemical analysis of 22 stars along thecolour-magnitude sequence of the interm...
Context. Open clusters are ideal test particles for studying the chemical evolution of the Galactic ...
International audienceWe present a detailed chemical analysis of 22 stars along the colour-magnitude...
International audienceContext. Classical chemical analyses may be affected by systematic errors that...
Spectroscopic determinations of the relative abundances of chemical elements produced in different n...
Context. Galactic open clusters have been long recognized as one of the best tools to investigate th...
We report on VLT/UVES high-resolution spectra of four members of the old metal-rich open cluster NGC...
We present chemical abundances for O, Na, Mg, Al, Si, Ca, Ti, and Fe in eight red giants and one tur...
We present a detailed chemical analysis of 22 stars along the colour–magnitude sequence of the inter...
Context. Classical chemical analyses may be affected by systematic errors that would cause observed...
Context. Galactic open clusters have been long recognized as one of the best tools to investigate th...
A detailed abundance analysis of 2 giants of the metal-rich bulge globular cluster NGC6553 was carri...
Recent theoretical yields and chemical evolution models demonstrate that intermediate-mass AGB stars...
We present detailed chemical abundance measurements for 45 globular clusters (GCs) associated with g...
International audienceAims: We present the abundance measurements of several elements (Fe, Ca, Na, N...
We present a detailed chemical analysis of 22 stars along thecolour-magnitude sequence of the interm...
Context. Open clusters are ideal test particles for studying the chemical evolution of the Galactic ...
International audienceWe present a detailed chemical analysis of 22 stars along the colour-magnitude...
International audienceContext. Classical chemical analyses may be affected by systematic errors that...
Spectroscopic determinations of the relative abundances of chemical elements produced in different n...
Context. Galactic open clusters have been long recognized as one of the best tools to investigate th...
We report on VLT/UVES high-resolution spectra of four members of the old metal-rich open cluster NGC...
We present chemical abundances for O, Na, Mg, Al, Si, Ca, Ti, and Fe in eight red giants and one tur...
We present a detailed chemical analysis of 22 stars along the colour–magnitude sequence of the inter...
Context. Classical chemical analyses may be affected by systematic errors that would cause observed...
Context. Galactic open clusters have been long recognized as one of the best tools to investigate th...
A detailed abundance analysis of 2 giants of the metal-rich bulge globular cluster NGC6553 was carri...
Recent theoretical yields and chemical evolution models demonstrate that intermediate-mass AGB stars...
We present detailed chemical abundance measurements for 45 globular clusters (GCs) associated with g...