Search

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation
Large resolution
Hi-Resolution Export to PDF

ALMA Observations of Magnetic Fields in the Massive Star-forming Region IRAS 18360-0537

  • Authors: Shixian Mo, Keping Qiu, Qizhou Zhang, Junhao Liu, Josep Miquel Girart, Hauyu Baobab Liu, Zhi-Yun Li, Shanghuo Li, Huei-Ru Vivien Chen

Shixian Mo et al 2026 The Astronomical Journal 172 .

  • Provider: AAS Journals

Caption: Figure 8.

Structure function for a center region of IRAS 18360. The measured angle dispersion is shown in black solid circles with the error bars. The best is shown by the blue dashed line. The vertical dashed line represents the beam size of the observations ∼1﹩\mathop{.}\limits^{\unicode{x02033}}﹩1 and the horizontal red dashed line is the predicted angle dispersion for a random field ∼52°.

Other Images in This Article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Copyright and Terms & Conditions

Additional terms of reuse