Showing 2022 · astro-ph.SRShow all

20 papers · 2 filters

astro-ph.SR2022★ 9 cited

The Gaia-ESO Survey: Probing the lithium abundances in old metal-rich dwarf stars in the Solar vicinity

M. L. L. Dantas, G. Guiglion, R. Smiljanic +14

We test a scenario in which radial migration could affect the Li abundance pattern of dwarf stars in the solar neighbourhood. This may confirm that the Li abundance in these stars…

astro-ph.SR2022★ 16 cited

Application of a magnetic-field-induced transition in Fe X to solar and stellar coronal magnetic field measurements

Yajie Chen, Wenxian Li, Hui Tian +3

Magnetic fields play a key role in driving a broad range of dynamic phenomena in the atmospheres of the Sun and other stars. Routine and accurate measurements of the magnetic field…

astro-ph.SR2022★ 39 cited

Comparative analysis of atmospheric parameters from high-resolution spectroscopic sky surveys: APOGEE, GALAH, Gaia-ESO

Viola Hegedűs, Szabolcs Mészáros, Paula Jofré +5

SDSS-IV APOGEE-2, GALAH and Gaia-ESO are high resolution, ground-based, multi-object spectroscopic surveys providing fundamental stellar atmospheric parameters and multiple element…

astro-ph.SR2022★ 25 cited

Connecting photometric and spectroscopic granulation signals with CHEOPS and ESPRESSO

S. Sulis, M. Lendl, H. Cegla +83

Stellar granulation generates fluctuations in photometric and spectroscopic data whose properties depend on the stellar type, composition, and evolutionary state. In this study, we…

astro-ph.SR2022★ 3 cited

The first r-process enhanced star confirmed to be a member of the Galactic bulge

R. Forsberg, R. M. Rich, N. Nieuwmunster +4

Aims. Stars with strong enhancements of r-process elements are rare and tend to be metal-poor, with generally [Fe/H] <-2 dex and found in the halo. In this work we aim to investiga…

astro-ph.SR2022★ 27 cited

The Galactic Chemical Evolution of phosphorus observed with IGRINS

G. Nandakumar, N. Ryde, M. Montelius +30

Phosphorus (P) is considered to be one of the key elements for life, making it an important element to look for in the abundance analysis of spectra of stellar systems. Yet, there…