| The Parallax and 3D Kinematics of Water Masers in the Massive Star-forming Region G034.43+0.24 | |
Mai,Xiaofeng1,2; Zhang,Bo1; Reid,M. J.3; Moscadelli,L.4; Xu,Shuangjing1,5; Sun,Yan1; Zhang,Jingdong1,2; Chen W(陈文)2,6 ; Wen,Shiming1; Luo,Qiuyi1,2; Menten,Karl M.7; Zheng,Xingwu8; Brunthaler,Andreas7; Xu,Ye9; Wang,Guangli1
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| 发表期刊 | The Astrophysical Journal
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| 2023-05-01 | |
| 卷号 | 949期号:1 |
| DOI | 10.3847/1538-4357/acc52a |
| 产权排序 | 第6完成单位 |
| 收录类别 | SCI |
| 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. |
| 资助项目 | Natural Science Foundation of China (NSFC)[U1831136] ; Natural Science Foundation of China (NSFC)[U2031212] ; Natural Science Foundation of China (NSFC)[11903079] ; Shanghai Astronomical Observatory[N-2020-06-09-005] ; ALMA |
| 项目资助者 | Natural Science Foundation of China (NSFC)[U1831136, U2031212, 11903079] ; Shanghai Astronomical Observatory[N-2020-06-09-005] ; ALMA |
| 语种 | 英语 |
| 学科领域 | 天文学 ; 恒星与银河系 ; 恒星形成与演化 |
| 文章类型 | Article |
| 出版者 | IOP Publishing Ltd |
| 出版地 | TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND |
| ISSN | 0004-637X |
| URL | 查看原文 |
| WOS记录号 | WOS:000992618500001 |
| WOS研究方向 | Astronomy & Astrophysics |
| WOS类目 | Astronomy & Astrophysics |
| 关键词[WOS] | INFRARED DARK CLOUD ; TRIGONOMETRIC PARALLAXES ; H2O MASERS ; ACCURACY ; EMISSION ; DISTANCE |
| 引用统计 | |
| 文献类型 | 期刊论文 |
| 条目标识符 | http://ir.ynao.ac.cn/handle/114a53/26075 |
| 专题 | 射电天文研究组 |
| 通讯作者 | Zhang,Bo |
| 作者单位 | 1.Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai 200030, People’s Republic of China; [email protected] 2.School of Astronomy and Space Sciences, University of Chinese Academy of Sciences, No. 19A Yuquan Road, Beijing 100049, People’s Republic of China 3.Center for Astrophysics ∣ Harvard & Smithsonian, 60 Garden Street, Cambridge, MA 02138, USA 4.INAF-Osservatorio Astrofisico di Arcetri, Largo E.Fermi 5, I-50125 Firenze, Italy 5.Korea Astronomy and Space Science Institute, 776 Daedeok-daero, Yuseong-gu, Daejeon 34055, Republic of Korea 6.Yunnan Observatories, Chinese Academy of Sciences, Kunming 650216, Yunnan, People’s Republic of China 7.Max-Plank-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, Germany 8.School of Astronomy and Space Science, Nanjing University, 22 Hankou Road, Nanjing 210093, People’s Republic of China 9.Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008, People’s Republic of China |
| 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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| The Parallax and 3D （2231KB） | 期刊论文 | 出版稿 | 开放获取 | CC BY-NC-SA | 浏览 请求全文 | |
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