We observed two main sequence stars in the globular cluster NGC 2808, using X-shooter. We selected one of the targets on the blue main sequence (bMS) and one on the red main sequence (rMS) and measured abundances for several light elements that are expected to be different in stars of first and second generations in globular clusters. The differences between the bMS and the rMS stars amply exceed the errors and is in agreement with a difference in products of hydrogen burning at high temperature. More data are required to put the findings on more solid basis and to try to distinguish between the different models proposed to explain the formation of globular clusters.2 page(s
Context. Abundance variations in moderately metal-rich globular clusters can give clues about the fo...
International audienceContext. Motivated by recent reports concerning the observation of limited enr...
Context. Motivated by recent reports concerning the observation of limited enrichment in He but exce...
We observed two main sequence stars in the globular cluster NGC 2808, using X-shooter. We selected o...
We observed two main sequence stars in the globular cluster NGC 2808, using X-shooter. We selected o...
We present the first chemical composition study of two unevolved stars in the globular cluster NGC 2...
We present the first chemical composition study of two unevolved stars in the globular cluster NGC 2...
We present the first chemical composition study of two unevolved stars in the globular cluster NGC 2...
Pseudo two-colour diagrams or Chromosome maps (ChM) indicate that NGC 2808 host five different stell...
Photometric investigations have revealed that Galactic globular clusters (GCs) exhibit internal meta...
High-precision HST photometry has revealed that the globular cluster (GC) NGC 2808 hosts a triple ma...
Context. Galactic globular clusters (GCs) are now known to host multiple populations displaying part...
none3siRecent photometric results have identified a new population among globular cluster stars. Thi...
We present the abundance analysis of stars from the tip of the red giant branch (RGB) to below the R...
We have used spectra obtained as part of the Science Verification program of the FLAMES multi-object...
Context. Abundance variations in moderately metal-rich globular clusters can give clues about the fo...
International audienceContext. Motivated by recent reports concerning the observation of limited enr...
Context. Motivated by recent reports concerning the observation of limited enrichment in He but exce...
We observed two main sequence stars in the globular cluster NGC 2808, using X-shooter. We selected o...
We observed two main sequence stars in the globular cluster NGC 2808, using X-shooter. We selected o...
We present the first chemical composition study of two unevolved stars in the globular cluster NGC 2...
We present the first chemical composition study of two unevolved stars in the globular cluster NGC 2...
We present the first chemical composition study of two unevolved stars in the globular cluster NGC 2...
Pseudo two-colour diagrams or Chromosome maps (ChM) indicate that NGC 2808 host five different stell...
Photometric investigations have revealed that Galactic globular clusters (GCs) exhibit internal meta...
High-precision HST photometry has revealed that the globular cluster (GC) NGC 2808 hosts a triple ma...
Context. Galactic globular clusters (GCs) are now known to host multiple populations displaying part...
none3siRecent photometric results have identified a new population among globular cluster stars. Thi...
We present the abundance analysis of stars from the tip of the red giant branch (RGB) to below the R...
We have used spectra obtained as part of the Science Verification program of the FLAMES multi-object...
Context. Abundance variations in moderately metal-rich globular clusters can give clues about the fo...
International audienceContext. Motivated by recent reports concerning the observation of limited enr...
Context. Motivated by recent reports concerning the observation of limited enrichment in He but exce...