output
19912026
Showing 2014 · astro-ph.GAShow all

15 papers · 2 filters

astro-ph.GA2014★ 56 cited

Characterizing the High-Velocity Stars of RAVE: The Discovery of a Metal-Rich Halo Star Born in the Galactic Disk

K. Hawkins, G. Kordopatis, G. Gilmore +21

We aim to characterize high-velocity (HiVel) stars in the solar vicinity both chemically and kinematically using the fourth data release of the RAdial Velocity Experiment (RAVE). W…

astro-ph.GA2014★ 67 cited

The Gaia-ESO Survey: Kinematics of seven Galactic globular clusters

C. Lardo, E. Pancino, M. Bellazzini +24

The Gaia-ESO survey is a large public spectroscopic survey aimed at investigating the origin and formation history of our Galaxy by collecting spectroscopy of representative sample…

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.GA2014★ 47 cited

The Gaia-ESO Survey: Extracting diffuse interstellar bands from cool star spectra, DIB-based interstellar medium line-of-sight structures at the kpc scale

L. Puspitarini, R. Lallement, C. Babusiaux +26

We study how diffuse interstellar bands (DIBs) measured toward distance-distributed target stars can be used to locate dense interstellar (IS) clouds in the Galaxy and probe a line…

astro-ph.GA2014★ 44 cited

Chemical Abundances of M giants in the Galactic Center: a Single Metal-Rich Population with Low [alpha/Fe]

N. Ryde, M. Schultheis

Context. The formation and evolution of the Milky Way bulge is still largely an unanswered question. One of the most essential observables needed in its modelling are the metallici…

astro-ph.GA2014★ 129 cited

The Gaia-ESO Survey: the chemical structure of the Galactic discs from the first internal data release

Š. Mikolaitis, V. Hill, A. Recio-Blanco +31

Most high-resolution spectroscopic studies of the Galactic discs were mostly confined to objects in the solar vicinity. Here we aim at enlarging the volume in which individual chem…