The metallicity distribution of G dwarfs in the solar neighbourhood and the chemical evolution of the Galaxy
文献类型:期刊论文
作者 | Chang, RX; Hou, JL; Fu, CQ |
刊名 | CHINESE ASTRONOMY AND ASTROPHYSICS
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出版日期 | 2000-10-01 |
卷号 | 24期号:4页码:444-452 |
关键词 | G dwarfs metallicity solar neighbourhood chemical evolution |
英文摘要 | Based on a new metallicity distribution for G dwarfs within 25 pc of the sun this paper discusses in detail four galactic chemical evolution models in an inhomogeneous interstellar medium. It is shown that both the so-called simple model and the collapse model deviate greatly from the observations, while the two models labelled PIE (Prompt Initial Enrichment) and PPY (Proportional Yield) not only give much better fit, but also alleviate the so-called G-dwarf problem. The indications are that the outer halo has little influence on the chemical evolution near the Sun. |
WOS标题词 | Science & Technology ; Physical Sciences |
类目[WOS] | Astronomy & Astrophysics |
研究领域[WOS] | Astronomy & Astrophysics |
关键词[WOS] | H-II REGIONS ; SPIRAL GALAXIES ; NEIGHBORHOOD ; ABUNDANCES ; STARS |
收录类别 | SCI |
语种 | 英语 |
WOS记录号 | WOS:000165799700005 |
源URL | [http://119.78.226.72/handle/331011/28261] ![]() |
专题 | 上海天文台_星系宇宙学重点实验室 |
作者单位 | 1.Chinese Acad Sci, Shanghai Observ, Shanghai 200030, Peoples R China 2.Chinese Acad Sci, Beijing Astron Observ, Young Astronomers Ctr, Beijing 100080, Peoples R China |
推荐引用方式 GB/T 7714 | Chang, RX,Hou, JL,Fu, CQ. The metallicity distribution of G dwarfs in the solar neighbourhood and the chemical evolution of the Galaxy[J]. CHINESE ASTRONOMY AND ASTROPHYSICS,2000,24(4):444-452. |
APA | Chang, RX,Hou, JL,&Fu, CQ.(2000).The metallicity distribution of G dwarfs in the solar neighbourhood and the chemical evolution of the Galaxy.CHINESE ASTRONOMY AND ASTROPHYSICS,24(4),444-452. |
MLA | Chang, RX,et al."The metallicity distribution of G dwarfs in the solar neighbourhood and the chemical evolution of the Galaxy".CHINESE ASTRONOMY AND ASTROPHYSICS 24.4(2000):444-452. |
入库方式: OAI收割
来源:上海天文台
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