The observed spiral structure of the Milky Way | |
Hou, L. G.![]() ![]() | |
刊名 | ASTRONOMY & ASTROPHYSICS
![]() |
2014-09-01 | |
卷号 | 569 |
关键词 | Galaxy: disk Galaxy: structure Galaxy: kinematics and dynamics HII regions ISM: clouds |
英文摘要 | Context. The spiral structure of the Milky Way is not yet well determined. The keys to understanding this structure are to increase the number of reliable spiral tracers and to determine their distances as accurately as possible. HII regions, giant molecular clouds (GMCs), and 6.7 GHz methanol masers are closely related to high mass star formation, and hence they are excellent spiral tracers. The distances for many of them have been determined in the literature with trigonometric, photometric, and/or kinematic methods. |
收录类别 | SCI |
语种 | 英语 |
WOS记录号 | WOS:000343092100087 |
内容类型 | 期刊论文 |
源URL | [http://ir.bao.ac.cn/handle/114a11/6661] ![]() |
专题 | 国家天文台_射电天文研究部 |
作者单位 | Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China |
推荐引用方式 GB/T 7714 | Hou, L. G.,Han, J. L.. The observed spiral structure of the Milky Way[J]. ASTRONOMY & ASTROPHYSICS,2014,569. |
APA | Hou, L. G.,&Han, J. L..(2014).The observed spiral structure of the Milky Way.ASTRONOMY & ASTROPHYSICS,569. |
MLA | Hou, L. G.,et al."The observed spiral structure of the Milky Way".ASTRONOMY & ASTROPHYSICS 569(2014). |
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