The Parallax and 3D Kinematics of Water Masers in the Massive Star-forming Region G034.43+0.24
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...
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IOP Publishing
2023-01-01
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Online Access: | https://doi.org/10.3847/1538-4357/acc52a |
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author | Xiaofeng Mai Bo Zhang M. J. Reid L. Moscadelli Shuangjing Xu Yan Sun Jingdong Zhang Wen Chen Shiming Wen Qiuyi Luo Karl M. Menten Xingwu Zheng Andreas Brunthaler Ye Xu Guangli Wang |
author_facet | Xiaofeng Mai Bo Zhang M. J. Reid L. Moscadelli Shuangjing Xu Yan Sun Jingdong Zhang Wen Chen Shiming Wen Qiuyi Luo Karl M. Menten Xingwu Zheng Andreas Brunthaler Ye Xu Guangli Wang |
author_sort | Xiaofeng Mai |
collection | DOAJ |
description | 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. |
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language | English |
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publishDate | 2023-01-01 |
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spelling | doaj.art-1c1bce1531df455aa5d6b32a7e5140b52023-09-03T13:17:00ZengIOP PublishingThe Astrophysical Journal1538-43572023-01-0194911010.3847/1538-4357/acc52aThe Parallax and 3D Kinematics of Water Masers in the Massive Star-forming Region G034.43+0.24Xiaofeng Mai0https://orcid.org/0000-0001-7573-0145Bo Zhang1https://orcid.org/0000-0003-1353-9040M. J. Reid2https://orcid.org/0000-0001-7223-754XL. Moscadelli3https://orcid.org/0000-0002-8517-8881Shuangjing Xu4https://orcid.org/0000-0003-2953-6442Yan Sun5https://orcid.org/0000-0002-8604-5394Jingdong Zhang6Wen Chen7https://orcid.org/0000-0002-5519-0628Shiming Wen8Qiuyi Luo9https://orcid.org/0000-0003-4506-3171Karl M. Menten10https://orcid.org/0000-0001-6459-0669Xingwu Zheng11Andreas Brunthaler12https://orcid.org/0000-0003-4468-761XYe Xu13https://orcid.org/0000-0001-5602-3306Guangli Wang14Shanghai Astronomical Observatory, Chinese Academy of Sciences , Shanghai 200030, People’s Republic of China ; zb@shao.ac.cn; School of Astronomy and Space Sciences, University of Chinese Academy of Sciences , No. 19A Yuquan Road, Beijing 100049, People’s Republic of ChinaShanghai Astronomical Observatory, Chinese Academy of Sciences , Shanghai 200030, People’s Republic of China ; zb@shao.ac.cnCenter for Astrophysics ∣ Harvard & Smithsonian , 60 Garden Street, Cambridge, MA 02138, USAINAF-Osservatorio Astrofisico di Arcetri , Largo E.Fermi 5, I-50125 Firenze, ItalyShanghai Astronomical Observatory, Chinese Academy of Sciences , Shanghai 200030, People’s Republic of China ; zb@shao.ac.cn; Korea Astronomy and Space Science Institute , 776 Daedeok-daero, Yuseong-gu, Daejeon 34055, Republic of KoreaShanghai Astronomical Observatory, Chinese Academy of Sciences , Shanghai 200030, People’s Republic of China ; zb@shao.ac.cnShanghai Astronomical Observatory, Chinese Academy of Sciences , Shanghai 200030, People’s Republic of China ; zb@shao.ac.cn; School of Astronomy and Space Sciences, University of Chinese Academy of Sciences , No. 19A Yuquan Road, Beijing 100049, People’s Republic of ChinaSchool of Astronomy and Space Sciences, University of Chinese Academy of Sciences , No. 19A Yuquan Road, Beijing 100049, People’s Republic of China; Yunnan Observatories, Chinese Academy of Sciences , Kunming 650216, Yunnan, People’s Republic of ChinaShanghai Astronomical Observatory, Chinese Academy of Sciences , Shanghai 200030, People’s Republic of China ; zb@shao.ac.cnShanghai Astronomical Observatory, Chinese Academy of Sciences , Shanghai 200030, People’s Republic of China ; zb@shao.ac.cn; School of Astronomy and Space Sciences, University of Chinese Academy of Sciences , No. 19A Yuquan Road, Beijing 100049, People’s Republic of ChinaMax-Plank-Institut für Radioastronomie , Auf dem Hügel 69, D-53121 Bonn, GermanySchool of Astronomy and Space Science, Nanjing University , 22 Hankou Road, Nanjing 210093, People’s Republic of ChinaMax-Plank-Institut für Radioastronomie , Auf dem Hügel 69, D-53121 Bonn, GermanyPurple Mountain Observatory, Chinese Academy of Sciences , Nanjing 210008, People’s Republic of ChinaShanghai Astronomical Observatory, Chinese Academy of Sciences , Shanghai 200030, People’s Republic of China ; zb@shao.ac.cnWe 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.https://doi.org/10.3847/1538-4357/acc52aMilky Way GalaxyStar formationTrigonometric parallaxInterstellar masers |
spellingShingle | Xiaofeng Mai Bo Zhang M. J. Reid L. Moscadelli Shuangjing Xu Yan Sun Jingdong Zhang Wen Chen Shiming Wen Qiuyi Luo Karl M. Menten Xingwu Zheng Andreas Brunthaler Ye Xu Guangli Wang The Parallax and 3D Kinematics of Water Masers in the Massive Star-forming Region G034.43+0.24 The Astrophysical Journal Milky Way Galaxy Star formation Trigonometric parallax Interstellar masers |
title | The Parallax and 3D Kinematics of Water Masers in the Massive Star-forming Region G034.43+0.24 |
title_full | The Parallax and 3D Kinematics of Water Masers in the Massive Star-forming Region G034.43+0.24 |
title_fullStr | The Parallax and 3D Kinematics of Water Masers in the Massive Star-forming Region G034.43+0.24 |
title_full_unstemmed | The Parallax and 3D Kinematics of Water Masers in the Massive Star-forming Region G034.43+0.24 |
title_short | The Parallax and 3D Kinematics of Water Masers in the Massive Star-forming Region G034.43+0.24 |
title_sort | parallax and 3d kinematics of water masers in the massive star forming region g034 43 0 24 |
topic | Milky Way Galaxy Star formation Trigonometric parallax Interstellar masers |
url | https://doi.org/10.3847/1538-4357/acc52a |
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