Information from the kinematics of F and G stars in the solar neighborhood | |
Chen, YQ![]() ![]() ![]() | |
刊名 | CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS
![]() |
2002-10-01 | |
卷号 | 2期号:5页码:419-428 |
关键词 | stars : kinematics Galaxy : evolution Galaxy : solar neighborhood |
英文摘要 | We have calculated the orbital parameters for 90 stars in Chen et al. and updated the kinematic data for stars in Edvardsson et al. by using the accurate Hipparcos parallaxes and proper motions, and recalculated the a-element abundances in Edvardsson et al. in a way consistent with Chen et al. The two sets of data are combined in a study of stellar populations and characteristics of F & G stars in the solar neighborhood. We confirm the result of Chen et al. that a distinguishable group of stars may belong to the thick disk rather than the thin disk. The ages for the stars are determined using the theoretical isochrones of VandenBerg et al. The age-metallicity relation is investigated for different subgroups according to distance from the sun and galactic orbital parameters. It is found that a mixing of stars with different orbital parameters significantly affect the age-metallicity relation for the disk. Stars with orbits confined to the solar circle all have metallicities [Fe/H] > -0.3 irrespective of their distances from the sun or from the Galactic plane. |
收录类别 | SCI |
语种 | 英语 |
WOS记录号 | WOS:000178799000005 |
内容类型 | 期刊论文 |
源URL | [http://ir.bao.ac.cn/handle/114a11/8514] ![]() |
专题 | 国家天文台_光学天文研究部 |
作者单位 | Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China |
推荐引用方式 GB/T 7714 | Chen, YQ,Zhao, G,Shi, JR. Information from the kinematics of F and G stars in the solar neighborhood[J]. CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS,2002,2(5):419-428. |
APA | Chen, YQ,Zhao, G,&Shi, JR.(2002).Information from the kinematics of F and G stars in the solar neighborhood.CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS,2(5),419-428. |
MLA | Chen, YQ,et al."Information from the kinematics of F and G stars in the solar neighborhood".CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS 2.5(2002):419-428. |
个性服务 |
查看访问统计 |
相关权益政策 |
暂无数据 |
收藏/分享 |
除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。
修改评论