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The Parallax and 3D Kinematics of Water Masers in the Massive Star-forming Region G034.43+0.24
Mai,Xiaofeng8,9; Zhang,Bo9; Reid,M. J.7; Moscadelli,L.6; Xu,Shuangjing5,9; Sun,Yan9; Zhang,Jingdong8,9; Chen W(陈文)4,8; Wen,Shiming9; Luo,Qiuyi8,9
刊名The Astrophysical Journal
2023-05-01
卷号949期号:1
ISSN号0004-637X
DOI10.3847/1538-4357/acc52a
产权排序第6完成单位
英文摘要

We report a measurement of the trigonometric parallax of 22 GHz water masers in the massive star-forming region G034.43+0.24 as part of the Bar and Spiral Structure Legacy Survey using the Very Long Baseline Array. The parallax is 0.330 ± 0.018 mas, corresponding to a distance of 3.03 ? 0.16 + 0.17 kpc. This locates G034.43+0.24 near the inner edge of the Sagittarius spiral arm and at one end of a linear distribution of massive young stars that cross nearly the full width of the arm. The measured three-dimensional motion of G034.43+0.24 indicates a near-circular Galactic orbit. The water masers display arc-like distributions, possibly bow shocks, associated with winds from one or more massive young stars.

学科主题天文学 ; 恒星与银河系 ; 恒星形成与演化
语种英语
出版者The American Astronomical Society
WOS记录号IOP:APJ_949_1_10
内容类型期刊论文
源URL[http://ir.ynao.ac.cn/handle/114a53/26074]  
专题云南天文台_射电天文研究组
通讯作者Zhang,Bo
作者单位1.Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008, People’s Republic of China
2.School of Astronomy and Space Science, Nanjing University, 22 Hankou Road, Nanjing 210093, People’s Republic of China
3.Max-Plank-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, Germany
4.Yunnan Observatories, Chinese Academy of Sciences, Kunming 650216, Yunnan, People’s Republic of China
5.Korea Astronomy and Space Science Institute, 776 Daedeok-daero, Yuseong-gu, Daejeon 34055, Republic of Korea
6.INAF-Osservatorio Astrofisico di Arcetri, Largo E.Fermi 5, I-50125 Firenze, Italy
7.Center for Astrophysics ∣ Harvard & Smithsonian, 60 Garden Street, Cambridge, MA 02138, USA
8.School of Astronomy and Space Sciences, University of Chinese Academy of Sciences, No. 19A Yuquan Road, Beijing 100049, People’s Republic of China
9.Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai 200030, People’s Republic of China; zb@shao.ac.cn
推荐引用方式
GB/T 7714
Mai,Xiaofeng,Zhang,Bo,Reid,M. J.,et al. The Parallax and 3D Kinematics of Water Masers in the Massive Star-forming Region G034.43+0.24[J]. The Astrophysical Journal,2023,949(1).
APA Mai,Xiaofeng.,Zhang,Bo.,Reid,M. J..,Moscadelli,L..,Xu,Shuangjing.,...&Wang,Guangli.(2023).The Parallax and 3D Kinematics of Water Masers in the Massive Star-forming Region G034.43+0.24.The Astrophysical Journal,949(1).
MLA Mai,Xiaofeng,et al."The Parallax and 3D Kinematics of Water Masers in the Massive Star-forming Region G034.43+0.24".The Astrophysical Journal 949.1(2023).
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