Showing 21–40 of 59 results
/ Date/ Name
Apr 29, 2003Is Praesepe really different from the coeval Hyades cluster? The XMM-Newton viewMar 11, 2002UVES Be observations of early-G dwarfs in old clustersAug 3, 2011Mixing at young ages: Beryllium abundances in cool main-sequence stars of the open clusters IC 2391 and IC 2602Jun 21, 2018Gaia-ESO Survey: INTRIGOSS - A new library of High Resolution Synthetic SpectraNov 23, 2020The Gaia-ESO Survey: Oxygen abundance in the Galactic thin and thick disksMar 19, 2021Light Elements in the UniverseSep 18, 2004On the potassium-rotation connection in late-type Alpha Persei starsMar 31, 2016The extent of mixing in stellar interiors: the open clusters Collinder 261 and Melotte 66Jul 12, 2000X-ray Emission From Nearby M-dwarfs: the Super-saturation PhenomenonJun 17, 2016The Gaia-ESO survey: Hydrogen lines in red giants directly trace stellar massMay 26, 2016Gaia FGK Benchmark Stars: New Candidates At Low-MetallicitiesAug 30, 2016CNO abundances and carbon isotope ratios in evolved stars of the open clusters NGC 2324, NGC 2477, and NGC 3960May 21, 2024WST -- Widefield Spectroscopic Telescope: Motivation, science drivers and top-level requirements for a new dedicated facilityAug 19, 2025Barium isotopic ratios in metal-poor stars: calibrating the method with globular clustersDec 16, 2024Modelling chemical clocks -- Theoretical evidences of the space and time evolution of [s/alpha] in the Galactic disc with Gaia-ESO surveyJan 18, 2009Enhanced production of barium in low-mass stars: evidence from open clustersFeb 16, 2000Ages of late spectral type Vega-like starsNov 29, 2019The Gaia-ESO Survey: Carbon abundance in the Galactic thin and thick disksMay 29, 2015Open clusters in the Gaia-ESO Survey tracing the chemical history of the Milky WayMay 12, 2009Chemical composition of the young open clusters IC2602 and IC2391