output
19952026
most citedThe Gaia mission

7.1k citations

Showing 2013 · astro-ph.GAShow all

6 papers · 2 filters

astro-ph.GA2013★ 47 cited

The Gaia-ESO Survey: Abundance ratios in the inner-disk open clusters Trumpler 20, NGC 4815, NGC 6705

L. Magrini, S. Randich, D. Romano +50

Open clusters are key tools to study the spatial distribution of abundances in the disk and their evolution with time. Using the first release of stellar parameters and abundances…

astro-ph.GA2013★ 16 cited

The distance to the young cluster NGC 7129 and its age

V. Straizys, M. Maskoliunas, R. P. Boyle +6

The dust cloud TGU H645 P2 and embedded in it young open cluster NGC 7129 are investigated using the results of medium-band photometry of 159 stars in the Vilnius seven-colour syst…

astro-ph.GA2013★ 10 cited

The open cluster NGC 7142: interstellar extinction, distance and age

V. Straizys, M. Maskoliunas, R. P. Boyle +4

The results of medium-band photometry of 1037 stars in the area of old open cluster NGC 7142 down to V = 20.1 mag in the Vilnius seven-colour system are presented. Photometric resu…

astro-ph.GA2013★ 8 cited

Stellar substructures in the solar neighbourhood. II. Abundances of neutron-capture elements in the kinematic Group 3 of the Geneva-Copenhagen survey

Edita Stonkutė, Gražina Tautvaišienė, Birgitta Nordström +1

The evolution of chemical elements in a galaxy is linked to its star formation history. Variations in star formation history are imprinted in the relative abundances of chemical el…

astro-ph.GA2013★ 27 cited

Red clump stars of the Milky Way - laboratories of extra-mixing

G. Tautvaišienė, G. Barisevičius, Y. Chorniy +2

In this work we present the main atmospheric parameters, carbon, nitrogen and oxygen abundances, and 12C/13C ratios determined in a sample of 28 Galactic clump stars. Abundances of…

astro-ph.GA2013★ 36 cited

Deriving physical parameters of unresolved star clusters. I. Age, mass, and extinction degeneracies

Philippe de Meulenaer, Donatas Narbutis, Tadas Mineikis +1

Context. Stochasticity and physical parameter degeneracy problems complicate the derivation of the parameters (age, mass, and extinction) of unresolved star clusters when using bro…