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Parallax of Star-forming Region G027.22+0.14
Bian,S. B.1,2; Xu,Y.1; Li,J. J.1; Wu,Y. W.3,4; Zhang,B.5; Chen,X.5,6; Li,Y. J.1; Lin,Z. H.1,2; Hao,C. J.1,2; Liu,D. J.1,2
2022-01-11
发表期刊The Astronomical Journal
ISSN0004-6256
卷号163期号:2
摘要Abstract Using the Very Long Baseline Array, we measured the trigonometric parallax and proper motions toward a 6.7 GHz methanol maser in the distant high-mass star-forming region G027.22+0.14. The distance of this source is determined to be 6.3 ? 0.5 + 0.6 kpc. Combining its Galactic coordinates, radial velocity, and proper motion, we assign G027.22+0.14 to the far portion of the Norma arm. The low peculiar motion and lower luminosity of G027.22+0.14 support the conjecture by Immer et al. that low-luminosity sources tend to have low peculiar motions.
DOI10.3847/1538-3881/ac3d90
语种英语
WOS记录号IOP:aj_163_2_54
出版者The American Astronomical Society
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文献类型期刊论文
条目标识符http://210.72.145.45/handle/361003/13924
专题守时理论与方法研究室
通讯作者Xu,Y.
作者单位1.Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210033, People’s Republic of China; xuye@pmo.ac.cn
2.School of Astronomy and Space Science, University of Science and Technology of China, Hefei 230026, People’s Republic of China
3.National Time Service Center, Key Laboratory of Precise Positioning and Timing Technology, Chinese Academy of Sciences, Xi’an 710600, People’s Republic of China
4.National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan
5.Shanghai Astronomical Observatory, 80 Nandan Road, Shanghai 200030, People’s Republic of China
6.Center for Astrophysics, Guangzhou University, Guangzhou 510006, People’s Republic of China
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GB/T 7714
Bian,S. B.,Xu,Y.,Li,J. J.,et al. Parallax of Star-forming Region G027.22+0.14[J]. The Astronomical Journal,2022,163(2).
APA Bian,S. B..,Xu,Y..,Li,J. J..,Wu,Y. W..,Zhang,B..,...&Liu,D. J..(2022).Parallax of Star-forming Region G027.22+0.14.The Astronomical Journal,163(2).
MLA Bian,S. B.,et al."Parallax of Star-forming Region G027.22+0.14".The Astronomical Journal 163.2(2022).
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