Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Centre National de la Recherche ScientifiqueFR1.3k papers
- Massachusetts Institute of TechnologyUS1.3k papers
- University of BristolGB1.3k papers
- University of Maryland, College ParkUS1.3k papers
- Peking UniversityCN1.3k papers
- European Organization for Nuclear ResearchCH1.3k papers
- RWTH Aachen UniversityDE1.3k papers
- Rutherford Appleton LaboratoryGB1.3k papers
- University of ZurichCH1.3k papers
- The Ohio State UniversityUS1.3k papers
- Université Libre de BruxellesBE1.3k papers
- California Institute of TechnologyUS1.3k papers
6 papers · 2 filters
On the metallicity dependance of the [Y/Mg] - age relation for solar type stars
S. Feltzing, L. M. Howes, P. J. McMillan +1
Several recent studies of Solar twins in the Solar neighbourhood have shown a tight correlation between various elemental abundances and age, in particular [Y/Mg]. If this relation…
CNO abundances and carbon isotope ratios in evolved stars of the open clusters NGC 2324, NGC 2477, and NGC 3960
Grazina Tautvaisiene, Arnas Drazdauskas, Angela Bragaglia +2
Our main aim is to determine carbon-to-nitrogen and carbon isotope ratios for evolved giants in the open clusters NGC 2324, NGC 2477, and NGC 3960, which have turn-off masses of ab…
The AMBRE Project: Constraining the lithium evolution in the Milky Way
G. Guiglion, P. de Laverny, A. Recio-Blanco +5
The chemical evolution of lithium in the Milky Way represents a major problem in modern astrophysics. Indeed, lithium is, on the one hand, easily destroyed in stellar interiors, an…
The Gaia-ESO survey: Metal-rich bananas in the bulge
Angus A. Williams, N. W. Evans, Matthew Molloy +25
We analyse the kinematics of giant stars in the direction of the Galactic bulge, extracted from the Gaia-ESO survey in the region $-10^\circ \lesssim \ell \lesssim 10^\…
The Gaia-ESO Survey: Probes of the inner disk abundance gradient
H. R. Jacobson, E. D. Friel, L. Jilkova +41
The nature of the metallicity gradient inside the solar circle (R_GC < 8 kpc) is poorly understood, but studies of Cepheids and a small sample of open clusters suggest that it stee…
The Gaia-ESO Survey: the selection function of the Milky Way field stars
E. Stonkute, S. E. Koposov, L. M. Howes +26
The Gaia-ESO Survey was designed to target all major Galactic components (i.e., bulge, thin and thick discs, halo and clusters), with the goal of constraining the chemical and dyna…