Image Details

Choose export citation format:

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 7.

Top panel: contour map of the total (Stokes I) dust emission and the magnetic field vectors (the black contours are the same as Figure 9) with the best family of functions shown as B-vectors (cyan bars: parabolic model; blue bars: Ewertowski model) at the same position as the measured values. Bottom panel: position angle (P.A.) distribution of the polarization vectors for the best-fit parabolic model and Ewertowski model.

Other Images in This Article
Copyright and Terms & Conditions

Additional terms of reuse