Add to ORKGA recent survey of a large sample of massive Galactic asymptotic giant branch (AGB) stars shows that significant overabundances of rubidium (up to 100 times solar) are present in these stars. Zirconium, on the other hand, is not enriched compared to the
Abstract–We demonstrate that a massive asymptotic giant branch (AGB) star is a good candidate as the...
We report the first spectroscopic identification of massive Galactic asymptotic giant branch (AGB) s...
Context. We previously explored the circumstellar effects on Rb and Zr abundances in a sample (21) o...
Context. A recent survey of a large sample of Galactic intermediate-mass (>3 M⊙) asymptotic giant br...
Context. A recent survey of a large sample of Galactic intermediate-mass (>3 M⊙) asymptotic giant br...
Context. A recent survey of a large sample of Galactic intermediate-mass (>3 M⊙) asymptotic giant br...
Context. Luminous Galactic OH/IR stars have been identified as massive (>4-5 M) asymptotic giant ...
International audienceLithium and zirconium abundances (the latter taken as representative of s-proc...
Context. Luminous Galactic OH/IR stars have been identified as massive (>4–5 M⊙) asymptotic giant br...
Context. Luminous Galactic OH/IR stars have been identified as massive (>4–5 M⊙) asymptotic giant br...
Lithium and zirconium abundances (the latter taken as representative of s-process enrichment) are de...
We present the main results derived from a chemical analysis carried out on a large sample of galact...
Lithium and zirconium abundances (the latter taken as representative of s-process enrichment) are de...
The asymptotic giant branch (AGB) is formed by low- and intermediate-mass stars (0.8 M⊙ < M < ...
Lithium and zirconium abundances (the latter taken as representative for s-process enrichment) are d...
Abstract–We demonstrate that a massive asymptotic giant branch (AGB) star is a good candidate as the...
We report the first spectroscopic identification of massive Galactic asymptotic giant branch (AGB) s...
Context. We previously explored the circumstellar effects on Rb and Zr abundances in a sample (21) o...
Context. A recent survey of a large sample of Galactic intermediate-mass (>3 M⊙) asymptotic giant br...
Context. A recent survey of a large sample of Galactic intermediate-mass (>3 M⊙) asymptotic giant br...
Context. A recent survey of a large sample of Galactic intermediate-mass (>3 M⊙) asymptotic giant br...
Context. Luminous Galactic OH/IR stars have been identified as massive (>4-5 M) asymptotic giant ...
International audienceLithium and zirconium abundances (the latter taken as representative of s-proc...
Context. Luminous Galactic OH/IR stars have been identified as massive (>4–5 M⊙) asymptotic giant br...
Context. Luminous Galactic OH/IR stars have been identified as massive (>4–5 M⊙) asymptotic giant br...
Lithium and zirconium abundances (the latter taken as representative of s-process enrichment) are de...
We present the main results derived from a chemical analysis carried out on a large sample of galact...
Lithium and zirconium abundances (the latter taken as representative of s-process enrichment) are de...
The asymptotic giant branch (AGB) is formed by low- and intermediate-mass stars (0.8 M⊙ < M < ...
Lithium and zirconium abundances (the latter taken as representative for s-process enrichment) are d...
Abstract–We demonstrate that a massive asymptotic giant branch (AGB) star is a good candidate as the...
We report the first spectroscopic identification of massive Galactic asymptotic giant branch (AGB) s...
Context. We previously explored the circumstellar effects on Rb and Zr abundances in a sample (21) o...