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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Main Authors: 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
Format: Article
Language:English
Published: IOP Publishing 2023-01-01
Series:The Astrophysical Journal
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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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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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