On the local stellar populations
文献类型：期刊论文
| 作者 | Fuhrmann, Klaus1,2; Chini, Rolf1,3; Kaderhandt, Lena1; Chen, Zhiwei1,4,5 |
| 刊名 | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
 |
| 出版日期 | 2017 |
| 卷号 | 464期号:3页码:2610-2621 |
| 关键词 | stars: fundamental parameters Galaxy: evolution Galaxy: formation solar neighbourhood Galaxy: stellar content |
| ISSN号 | 0035-8711 |
| DOI | 10.1093/mnras/stw2526 |
| 通讯作者 | Fuhrmann, Klaus(klaus@ing.iac.es) |
| 英文摘要 | We present a study of the local stellar populations from a volume-complete all-sky survey of the about 500 bright stars with distances less than 25 pc and down to main-sequence effective temperatures T-eff >= 5300 K. The sample is dominated by a 93 per cent fraction of Population I stars, only 22 sources (5 per cent) are Population II stars, and 9 sources (2 per cent) are intermediate-disc stars. No source belongs to the halo. By following the mass of the stars instead of their light, the resulting subset of 136 long-lived stars distributes as 22 (16.2 per cent): 6 (4.4 per cent): 108 (79.4 per cent) for the Population II: intermediate disc: Population I, respectively. Along with the much larger scaleheight reached by Population II, this unbiased census of long-lived stars provides plain evidence for a starburst epoch in the early Milky Way, with the formation of a massive, rotationally supported, and dark Population II. The same conclusion arises from the substantial early chemical enrichment levels, exemplified here by the elements magnesium and iron, as it arises also from the local Population II white dwarfs. The kinematics, metallicity distribution functions, star formation rates, age-metallicity relations, the inventory of young stars, and the occurrence of blue straggler stars are discussed. A potentially new aspect of the survey is the possibility for substructure among the local Population II stars that may further subdivide into metal-poor and metal-rich sources. |
| WOS关键词 | SOLAR-TYPE STARS ; COOL DWARF STARS ; NEARBY STARS ; CHEMICAL EVOLUTION ; METAL ABUNDANCES ; WHITE-DWARFS ; MILKY-WAY ; METALLICITY DISTRIBUTION ; SPECTROSCOPIC SURVEY ; BINARY-SYSTEMS |
| WOS研究方向 | Astronomy & Astrophysics |
| 语种 | 英语 |
| WOS记录号 | WOS:000393647600008 |
| 出版者 | OXFORD UNIV PRESS |
| 源URL | [http://libir.pmo.ac.cn/handle/332002/23300]  |
| 专题 | 中国科学院紫金山天文台 |
| 通讯作者 | Fuhrmann, Klaus |
| 作者单位 | 1.Ruhr Univ Bochum, Astron Inst, Univ Str 150, D-44801 Bochum, Germany 2.Isaac Newton Grp Telescopes, Apartado 321, E-38700 Santa Cruz De La Palma, Spain 3.Univ Catolica Norte, Inst Astron, Ave Angamos 0610,Casilla 1280, Antofagasta, Chile 4.Chinese Acad Sci, Purple Mt Observ, 2 West Beijing Rd, Nanjing 210008, Jiangsu, Peoples R China 5.Chinese Acad Sci, Key Lab Radio Astron, 2 West Beijing Rd, Nanjing 210008, Jiangsu, Peoples R China |
| 推荐引用方式 GB/T 7714 | Fuhrmann, Klaus,Chini, Rolf,Kaderhandt, Lena,et al. On the local stellar populations[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2017,464(3):2610-2621. |
| APA | Fuhrmann, Klaus,Chini, Rolf,Kaderhandt, Lena,&Chen, Zhiwei.(2017).On the local stellar populations.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,464(3),2610-2621. |
| MLA | Fuhrmann, Klaus,et al."On the local stellar populations".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 464.3(2017):2610-2621. |
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来源：紫金山天文台
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