NTSC-IR  > 高精度时间传递与精密测定轨研究室
thespiralstructureofthemilkyway
Xu Ye1; Hou Ligang2; Wu Yuanwei3
2018
发表期刊researchinastronomyandastrophysics
ISSN1674-4527
卷号18期号:12页码:9
摘要The morphology and kinematics of the spiral structure of the Milky Way are long-standing problems in astrophysics. In this review we firstly summarize variousmethodswith different tracers used to solve this puzzle. The astrometry of Galactic sources is gradually alleviating this difficult situation caused mainly by large distance uncertainties, as we can currently obtain accurate parallaxes (a few mu as) and proper motions (approximate to 1 kms(-1)) by using Very Long Baseline Interferometry (VLBI). On the other hand, the Gaia mission is providing the largest, uniform sample of parallaxes for O-type stars in the entire Milky Way. Based upon the VLBI maser and Gaia O-star parallax measurements, nearby spiral structures of the Perseus, Local, Sagittarius and Scutum Arms are determined in unprecedented detail. Meanwhile, we estimate fundamental Galactic parameters of the distance to the Galactic center, R-0, to be 8.35 +/- 0.18 kpc, and circular rotation speed at the Sun, theta(0), to be 240 +/- 10 kms(-1). We found kinematic differences between O stars and interstellar masers: the O stars, on average, rotate faster, > 8 kms(-1) than maser-traced high-mass star forming regions.
语种英语
资助项目[MOST] ; [NSFC] ; [CAS] ; [Youth Innovation Promotion Association of CAS] ; [Key Laboratory for Radio Astronomy, CAS] ; [Open Project Program of the Key Laboratory of FAST, NAOC, CAS]
文献类型期刊论文
条目标识符http://210.72.145.45/handle/361003/9754
专题高精度时间传递与精密测定轨研究室
作者单位1.中国科学院紫金山天文台
2.中国科学院国家天文台
3.中国科学院国家授时中心
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GB/T 7714
Xu Ye,Hou Ligang,Wu Yuanwei. thespiralstructureofthemilkyway[J]. researchinastronomyandastrophysics,2018,18(12):9.
APA Xu Ye,Hou Ligang,&Wu Yuanwei.(2018).thespiralstructureofthemilkyway.researchinastronomyandastrophysics,18(12),9.
MLA Xu Ye,et al."thespiralstructureofthemilkyway".researchinastronomyandastrophysics 18.12(2018):9.
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