期刊文献+
共找到1篇文章
< 1 >
每页显示 20 50 100
Elliptical distortion of the Milky Way's rotation traced by high-mass star-forming regions
1
作者 Ping-Jie Ding Zi Zhu Jia-Cheng Liu 《Research in Astronomy and Astrophysics》 SCIE CAS CSCD 2017年第11期85-94,共10页
The gravitational potential of the Milky Way is non-axisymmetric, caused by a bar or triaxial halo, which dominates elliptical rotation of the Milky Way. Employing a likelihood analysis, we exploit the astrometric dat... The gravitational potential of the Milky Way is non-axisymmetric, caused by a bar or triaxial halo, which dominates elliptical rotation of the Milky Way. Employing a likelihood analysis, we exploit the astrometric data of masers thoroughly and constrain the elliptical rotation of the Galaxy. Masers in high-mass star-forming regions, observed by VLBA, are more distant tracers than stars observed in the optical bandpass, and thus are more appropriate for studying the global feature of the Milky Way's rotation. A clear elliptical potential of the Milky Way is detected, with an ellipticity of ε0-0.09 at the Sun, and the ellipticity increases towards the outer disk. The minor axis of the elliptical potential (the major axis of the rotation orbit) is found to be near the Sun with a displacement of -32°. Based on the rotation model assumed for an elliptical potential, we also make a kinematical calibration of the Galactocentric distance of the Sun, which gives R0 = 7.63±0.34 kpc. 展开更多
关键词 astrometry -- Galaxy: fundamental parameters -- Galaxy: kinematics and dynamics --methods: data analysis
下载PDF
上一页 1 下一页 到第
使用帮助 返回顶部