Influence of alpha-enhancement on effective temperatures of hot subdwarfs | |
Guo JP(郭建坡)1,2,3; Zhang FH(张奉辉)1,2; Zhang XF(张先飞)1,2,3; Han ZW(韩占文)1,2; Guo, JP (reprint author), Chinese Acad Sci, Natl Astron Observ, Yunnan Observ, Kunming 650011, Peoples R China. | |
发表期刊 | ASTROPHYSICS AND SPACE SCIENCE |
2010-10 | |
卷号 | 329期号:1-2页码:15-18 |
DOI | 10.1007/s10509-010-0291-4 |
产权排序 | 第1完成单位 |
收录类别 | SCI |
关键词 | Stars: Abundances Stars: Subdwarfs Stars: Horizontal-branch |
摘要 | Observations of metal elements in some halo or bulge globular clusters and in some elliptical galaxies have shown the alpha-enhancement phenomenon. Hot subdwarfs are important stars, e.g., they are important sources of far-ultraviolet light in the Galaxy and have successfully been used to explain the UV-upturn in elliptical galaxies. Therefore, we try to study the impacts of alpha-enhancement on hot subdwarfs. In our calculation, the value of the metallicity is 0.02, all the core masses of hot subdwarfs are 0.475 M (aS (TM)), and the envelope masses of the hot subdwarfs are 0.001, 0.005 and 0.016 M (aS (TM)), respectively. We find that the influences of alpha-enhancement on luminosity and evolutionary age of hot subdwarfs are not visible. But alpha-enhancement can make the effective temperatures of hot subdwarfs become higher, and the thicker their envelopes are, the more obvious this influence is. |
项目资助者 | National Natural Science Foundation of China [10773026, 10821061, 2007CB815406] ; Chinese Academy of Sciences [KJCX2-YW-T24] ; Yunnan Natural Science Foundation [06GJ061001] |
语种 | 英语 |
学科领域 | Astronomy & Astrophysics |
文章类型 | Article |
ISSN | 0004-640X |
URL | 查看原文 |
WOS记录号 | WOS:000282823200004 |
WOS研究方向 | Astronomy & Astrophysics |
WOS类目 | Astronomy & Astrophysics |
关键词[WOS] | STELLAR EVOLUTION ; ELLIPTIC GALAXIES ; GLOBULAR-CLUSTERS ; MODELS ; STARS ; OPACITIES ; ISOCHRONES ; INDEXES ; SYSTEMS ; CARBON |
引用统计 | |
文献类型 | 期刊论文 |
条目标识符 | http://ir.ynao.ac.cn/handle/114a53/4486 |
专题 | 大样本恒星演化研究组 中国科学院天体结构与演化重点实验室 |
通讯作者 | Guo, JP (reprint author), Chinese Acad Sci, Natl Astron Observ, Yunnan Observ, Kunming 650011, Peoples R China. |
作者单位 | 1.National Astronomical Observatories/Yunnan Observatory, Chinese Academy of Sciences, Kunming, 650011, P.R. China 2.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming, 650011, P.R. China 3.Graduate School of the Chinese Academy of Sciences, Beijing, 100049, P.R. China |
第一作者单位 | 中国科学院云南天文台 |
推荐引用方式 GB/T 7714 | Guo JP,Zhang FH,Zhang XF,et al. Influence of alpha-enhancement on effective temperatures of hot subdwarfs[J]. ASTROPHYSICS AND SPACE SCIENCE,2010,329(1-2):15-18. |
APA | Guo JP,Zhang FH,Zhang XF,Han ZW,&Guo, JP .(2010).Influence of alpha-enhancement on effective temperatures of hot subdwarfs.ASTROPHYSICS AND SPACE SCIENCE,329(1-2),15-18. |
MLA | Guo JP,et al."Influence of alpha-enhancement on effective temperatures of hot subdwarfs".ASTROPHYSICS AND SPACE SCIENCE 329.1-2(2010):15-18. |
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