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East Asian VLBI Network Astrometry Toward the Star-forming Region G040.96+02.48 in the Extreme Outer Galaxy

  • Authors: Xianjin Shen, Zehao Lin, Nobuyuki Sakai, Ye Xu, Shuaibo Bian, Yuanwei Wu, Yan Sun, Dejian Liu, Jingjing Li, Bo Zhang, Shuangjing Xu, Tomoaki Oyama, Chungsik Oh, Wu Jiang, Lang Cui, Pengfei Jiang, Guanghui Li, Mareki Honma, Se-Jin Oh, Zhi-Qiang Shen, Na Wang

Xianjin Shen et al 2026 The Astronomical Journal 171 .

  • Provider: AAS Journals

Caption: Figure 5.

Spatial distributions of three most distant star-forming regions with precise distance measurements projected onto the Galactic plane. The sources shown in clockwise order are G040.96+02.48 (this work), G034.84−00.95 (N. Sakai et al. 2023), and G007.47+0.06 (A. Sanna et al. 2017). The yellow arrow shows the peculiar motion vector of star-forming region G040.96+02.48. A velocity scale of 50 km s−1 is indicated in the plot. The background is a new artist’s impression of the Milky Way credited by Xing-Wu Zheng & Mark Reid BeSSeL/NJU/CFA. The Sun’s position is at (0, 8.15) kpc, while the Galactic Center is at (0.0, 0.0) kpc.

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