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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
DOI10.1007/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
ISSN0004-640X
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
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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
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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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