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20022026
most citedA stellar relic from the early Milky Way

527 citations · 2.6k across the 21 of their papers we have counts for

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11 papers · 1 filter

astro-ph.SR2026

Evidence for elemental diffusion in the eclipsing binary star AI Phoenicis

Pierre F. L. Maxted, Nicholas Storm, Andreas J. Korn +7

AI Phe is an eclipsing binary star with an orbital period of 24.6 days for which the surface gravity and effective temperature are known from direct measurements to very high preci…

astro-ph.SR2026

Stellar masses and ages in Gaia Data Release 4 from the Final Luminosity Age Mass Estimator algorithm

Orlagh L. Creevey, Laia Casamiquela, Yveline Lebreton +23

The masses and ages of stars are key quantities for understanding exoplanetary, stellar, and galactic evolution. In the context of Gaia, these parameters provide insights into the…

astro-ph.SR2018★ 42 cited

The Gaia-ESO Survey: properties of newly discovered Li-rich giants

R. Smiljanic, E. Franciosini, A. Bragaglia +41

We report 20 new lithium-rich giants discovered within the Gaia-ESO Survey, including the first Li-rich giant with evolutionary stage confirmed by CoRoT data. Atmospheric parameter…

astro-ph.SR2018★ 66 cited

The Gaia-ESO survey: impact of extra-mixing on C- and N-abundances of giant stars

N. Lagarde, C. Reylé, A. C. Robin +30

The GES survey using FLAMES at the VLT has obtained high-resolution UVES spectra for a large number of giant stars, allowing a determination of the abundances of the key chemical e…

astro-ph.SR2017★ 12 cited

Sun-like stars unlike the Sun: Clues for chemical anomalies of cool stars

V. Adibekyan, E. Delgado-Mena, S. Feltzing +11

We present a summary of the splinter session "Sun-like stars unlike the Sun" that was held on 09 June 2016 as part of the Cool Stars 19 conference (Uppsala, Sweden). We discussed t…

astro-ph.SR2015★ 20 cited

Stellar science from a blue wavelength range - A possible design for the blue arm of 4MOST

C. J. Hansen, H. -G. Ludwig, W. Seifert +12

From stellar spectra, a variety of physical properties of stars can be derived. In particular, the chemical composition of stellar atmospheres can be inferred from absorption line…