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19982026
most citedChemical Evolution of the Magellanic Clouds: analytical models

232 citations · 3.1k across the 81 of their papers we have counts for

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Showing 2014Show all

7 papers · 1 filter

astro-ph.SR2014★ 61 cited

The Gaia-ESO Survey: CNO abundances in the open clusters Trumpler 20, NGC 4815, and NGC 6705

G. Tautvaišienė, A. Drazdauskas, Š. Mikolaitis +30

Aim of this work is to determine C, N, and O abundances in stars of Galactic open clusters of the Gaia-ESO survey and to compare the observed abundances with those predicted by cur…

astro-ph.GA2014★ 11 cited

The Gaia-ESO Survey: α-abundances of metal-poor stars

R. Jackson-Jones, P. Jofré, K. Hawkins +21

We performed a detailed study of the ratio of low-α to high-α stars in the Galactic halo as observed by the Gaia-ESO Survey. Using a sample of 381 metal-poor stars from the second…

astro-ph.SR2014★ 227 cited

Gaia-ESO Survey: The analysis of high-resolution UVES spectra of FGK-type stars

R. Smiljanic, A. J. Korn, M. Bergemann +99

The Gaia-ESO Survey is obtaining high-quality spectroscopic data for about 10^5 stars using FLAMES at the VLT. UVES high-resolution spectra are being collected for about 5000 FGK-t…

astro-ph.SR2014★ 80 cited

The Gaia-ESO Survey: Stellar content and elemental abundances in the massive cluster NGC 6705

T. Cantat-Gaudin, A. Vallenari, S. Zaggia +52

Chemically inhomogeneous populations are observed in most globular clusters, but not in open clusters. Cluster mass seems to play a key role in the existence of multiple population…

astro-ph.SR2014★ 42 cited

The Gaia-ESO Survey: metallicity of the Chamaeleon I star forming region

L. Spina, S. Randich, F. Palla +37

Context. Recent metallicity determinations in young open clusters and star-forming regions suggest that the latter may be characterized by a slightly lower metallicity than the Sun…

astro-ph.SR2014★ 9 cited

Stellar substructures in the solar neighbourhood. III. Kinematic group 2 in the Geneva-Copenhagen survey

R. Ženovienė, G. Tautvaišienė, B. Nordström +1

From correlations between orbital parameters, several new coherent groups of stars were recently identified in the Galactic disc and suggested to correspond to remnants of disrupte…