output
19912026
most citedObservation of a new particle in the search for the Standard Model Higgs boson with the ATLAS detector at the LHC

10.9k citations

Showing 2014 · astro-ph.SRShow all

16 papers · 2 filters

astro-ph.SR2014

The SAGA so far: reading the history of the Galaxy with asteroseismology

Luca Casagrande, Victor Silva Aguirre, Aldo M. Serenelli +3

Asteroseismology has the capability of delivering stellar properties which would otherwise be inaccessible, such as radii, masses and thus ages of stars. When this information is c…

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.SR2014★ 74 cited

On the Numerical Treatment and Dependence of Thermohaline Mixing in Red Giants

John Lattanzio, Lionel Siess, Ross Church +5

In recent years much interest has been shown in the process of thermohaline mixing in red giants. In low and intermediate mass stars this mechanism first activates at the position…

astro-ph.SR2014★ 7 cited

Systematic trend of water vapour absorption in red giant atmospheres revealed by high resolution TEXES 12 micron spectra

N. Ryde, J. Lambert, M. Farzone +5

The structures of the outer atmospheres of red giants are very complex. The notion of large optically thick molecular spheres around the stars (MOLspheres) has been invoked in orde…

astro-ph.SR2014★ 73 cited

The Gaia-ESO Survey: the most metal-poor stars in the Galactic bulge

L. Howes, M. Asplund, A. R. Casey +39

We present the first results of the EMBLA survey (Extremely Metal-poor BuLge stars with AAOmega), aimed at finding metal-poor stars in the Milky Way bulge, where the oldest stars s…

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…