中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
The Impact of Diffusion and Turbulent Mixing on Chemical Abundance Variations in the Open Cluster NGC 2420

文献类型:期刊论文

作者Guo, Fei2; Li XF(李雪峰)3; Li Y(李焱)1,3,4,5
刊名ASTROPHYSICAL JOURNAL
出版日期2026-02-20
卷号998期号:2
ISSN号0004-637X
DOI10.3847/1538-4357/ae3daf
产权排序第2完成单位
文献子类Article
英文摘要The mixing of material in stellar envelopes critically determines surface elemental abundances. A well-established tension remains between theoretical models and observational data for stars near the main-sequence turn-off. Resolving this issue requires developing a more physically complete treatment of material mixing, likely arising from processes inadequately represented in standard stellar models. This paper discusses four mixing mechanisms, including convection, convective overshooting, radiative diffusivity, and atomic diffusion, with particular focus on their combined impact on the surface elemental abundances of stars in the open cluster NGC 2420 during stellar evolution. We find that changes in the surface elemental abundances depend on the initial mass of the star and its evolutionary stage. The addition of extra mixing (radiative diffusivity) can resolve the issue of pure hydrogen atmospheres that arises for stars with masses greater than 1.35 M circle dot. Our best-fitting model (Con+Ov+Diff) with a moderate overshoot parameter fov similar to 0.0174 reproduces the observed abundance dip in NGC 2420, confirming atomic diffusion as the key mechanism and supporting a cluster age of similar to 2.5 Gyr.
学科主题天文学 ; 恒星与银河系
URL标识查看原文
出版地No.2 The Distillery, Glassfields, Avon Street, Bristol, ENGLAND
WOS关键词RED GIANT STARS ; ATOMIC DIFFUSION ; CONVECTIVE BOUNDARIES ; ELEMENT DIFFUSION ; MAIN-SEQUENCE ; MODULES ; EVOLUTION ; SUBGIANT ; ROTATION ; TURNOFF
资助项目Yunnan Province Foundation[202301AU070160]
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:001694241500001
出版者IOP Publishing Ltd
资助机构Yunnan Province Foundation[202301AU070160]
版本出版稿
源URL[http://ir.ynao.ac.cn/handle/114a53/28929]  
专题云南天文台_恒星物理研究组
通讯作者Guo, Fei
作者单位1.Center for Astronomical Mega-Science, Chinese Academy of Sciences, Beijing 100012, People’s Republic of China
2.Yunnan Normal University, Kunming 650500, People’s Republic of China; guofei@ynnu.edu.cn;
3.Yunnan Observatories, Chinese Academy of Sciences, P.O.Box110, Kunming 650216, People’s Republic of China;
4.University of Chinese Academy of Sciences, Beijing 100049, People’s Republic of China;
5.Key Laboratory for Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, P.O.Box110, Kunming 650216, People’s Republic of China;
推荐引用方式
GB/T 7714
Guo, Fei,Li XF,Li Y. The Impact of Diffusion and Turbulent Mixing on Chemical Abundance Variations in the Open Cluster NGC 2420[J]. ASTROPHYSICAL JOURNAL,2026,998(2).
APA Guo, Fei,李雪峰,&李焱.(2026).The Impact of Diffusion and Turbulent Mixing on Chemical Abundance Variations in the Open Cluster NGC 2420.ASTROPHYSICAL JOURNAL,998(2).
MLA Guo, Fei,et al."The Impact of Diffusion and Turbulent Mixing on Chemical Abundance Variations in the Open Cluster NGC 2420".ASTROPHYSICAL JOURNAL 998.2(2026).

入库方式: OAI收割

来源:云南天文台

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