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arXiv 2609.37613astro-ph.SRastro-ph.GA

三颗新的极贫金属恒星(含一颗CEMP-s恒星)的丰度分析

Abundance analysis of three new extremely metal-poor stars, including one CEMP-s star

P. François, T. Suda, S. Wanajo, E. Caffau, P. Bonifacio, W. Aoki, S. Yamada, M. Y. Fujimoto

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中文总结 AI 辅助

基于斯巴鲁HDS光谱,对三颗极贫金属恒星进行丰度分析,确认其性质,发现一颗具有最高[Mg/Fe]的CEMP-s恒星,并利用视向速度和盖亚数据确定其银河系轨道与运动学归属。

中文摘要 AI 辅助

我们利用斯巴鲁望远镜上的高色散光谱仪(HDS)获得的光谱,对三颗极贫金属(EMP)恒星进行了详细的丰度分析。目的是观测从斯隆数字巡天(SDSS)中选出的EMP候选恒星样本,并确定其详细的化学组成。使用斯巴鲁望远镜上的HDS对三颗暗的转向点恒星进行了高分辨率光谱观测。我们采用标准1D模型计算了多种元素(Li、C、Mg、Ca、Sr和Ba)的丰度。我们分析的恒星金属丰度[Fe/H]在-3.02到-3.57 dex之间。我们还测量了精确的视向速度,结合盖亚天体测量数据,使我们能够计算恒星的作用量和银河系轨道。我们的分析证实这些恒星是真正的EMP恒星。其中一颗(SDSS J074238.68+470537.0)可归类为CEMP-s恒星,其[Mg/Fe]比值是迄今在转向点CEMP-s恒星中测得最高的,[Mg/Fe]=1.85 dex。对于恒星SDSS J012630.30+073029.3([Fe/H]=-3.02 dex),我们明确探测到锂,A(Li)=2.05。在运动学上,SDSS J214340.08-002835.5是一颗厚盘恒星,而另外两颗属于晕族,是盖亚-香肠-恩克拉多斯(Gaia-Sausage-Enceladus)的候选成员。

英文摘要

We report a detailed abundance analysis of three extremely metal-poor (EMP) stars thanks to spectra obtained with the high-dispersion spectrograph (HDS) at the Subaru telescope. The aim is to observe a sample of EMP candidate stars selected from the Sloan Digital Sky Survey (SDSS) and determine their detailed chemical composition. High-resolution spectra of three faint turn-off stars using HDS on the Subaru telescope were acquired.We used standard 1D models to compute the abundances of several elements (Li, C, Mg, Ca, Sr, and Ba). The stars we analysed have a metallicity [Fe/H] of between -3.02 and -3.57 dex. We also measured accurate radial velocities that, coupled with the Gaia astrometric data, allowed us to compute actions and Galactic orbits for the stars. Our analysis confirms that the stars are genuine EMP stars. One of them (SDSS J074238.68 +470537.0) can be classified as a CEMP-s star with the highest [Mg/Fe] ratio ever measured in a turn-off CEMP-s star with [Mg/Fe] = 1.85 dex. For the star SDSS J012630.30+073029.3 ([Fe/H]= -3.02 dex), we have a clear detection of lithium with A(Li) = 2.05. Kinematically, SDSS J214340.08-002835.5 is a thick-disc star, while the other two belong to the halo and are candidate members of the Gaia- Sausage-Enceladus.

发表机构

  • LIRA, Observatoire de Paris, Université PSL, Sorbonne Université, Université Paris CitC), CY Cergy Paris Université, CNRS(巴黎天文台 LIRA 实验室,巴黎文理研究大学,索邦大学,巴黎西岱大学,塞吉-蓬图瓦兹大学,法国国家科学研究中心)
  • UPJV, Université de Picardie Jules Verne(亚眠皮卡第儒勒·凡尔纳大学)
  • Department of Liberal Arts, Tokyo University of Technology(东京工业大学人文学部)
  • Research Center for the Early Universe, The University of Tokyo(东京大学宇宙早期研究数据中心)
  • Department of Astronomy, Faculty of Science, Tohoku University(东北大学理学部天文学科)
  • National Observatory of Japan(日本国立天文台)
  • Faculty of Science, Hokkaido University(北海道大学理学部)

机构由 AI 辅助整理,请以论文原文为准。

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