{ "id": "2407.11572", "version": "v1", "published": "2024-07-16T10:23:29.000Z", "updated": "2024-07-16T10:23:29.000Z", "title": "Discovery of an Extremely r-process-enhanced Thin-disk Star with [Eu/H] = +0.78", "authors": [ "Xiao-Jin Xie", "Jianrong Shi", "Hong-Liang Yan", "Tian-Yi Chen", "Carlos Allende Prieto", "Timothy C. Beers", "Shuai Liu", "Chun-Qian Li", "Ming-Yi Ding", "Yao-Jia Tang", "Ruizhi Zhang", "Renjing Xie" ], "comment": "5 figures, 3 tables", "categories": [ "astro-ph.SR", "astro-ph.GA" ], "abstract": "Highly r-process-enhanced stars are rare and usually metal-poor ([Fe/H] < - 1.0), and mainly populate the Milky Way halo and dwarf galaxies. This study presents the discovery of a relatively bright (V = 12.72), highly r-process-enhanced (r-II) star ([Eu/Fe] = +1.32, [Ba/Eu] = - 0.95), LAMOST J020623.21 + 494127.9. This star was selected from the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) medium-resolution (R ~ 7500) spectroscopic survey; follow-up high-resolution (R ~ 25,000) observations were conducted with the High Optical Resolution Spectrograph (HORuS) installed on the Gran Telescopio Canarias (GTC). The stellar parameters (${T_{\\rm eff}}$ = 4130 K, $\\rm log\\,g $ = 1.52, $ \\rm[Fe/H] $ = $ - $0.54, $\\xi$ = 1.80 $ \\rm{km\\,{s^{-1}}} $) have been inferred taking into account non-local thermodynamic equilibrium (NLTE) effects. The abundances of [Ce/Fe], [Pr/Fe], and [Nd/Fe] are +0.19, +0.65 and +0.64, respectively, relatively low compared to the Solar r-process pattern normalized to Eu. This star has a high metallicity ([Fe/H] = - 0.54) compared to most other highly r-process-enhanced stars, and has the highest measured abundance ratio of Eu to H ([Eu/H] = +0.78). It is classified as a thin-disk star based on its kinematics, and does not appear to belong to any known stream or dwarf galaxy.", "revisions": [ { "version": "v1", "updated": "2024-07-16T10:23:29.000Z" } ], "analyses": { "keywords": [ "extremely r-process-enhanced thin-disk star", "area multi-object fiber spectroscopic telescope", "large sky area multi-object fiber", "sky area multi-object fiber spectroscopic" ], "note": { "typesetting": "TeX", "pages": 0, "language": "en", "license": "arXiv", "status": "editable" } } }