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Formation of the SDC13 Hub-filament System: A Cloud–Cloud Collision Imprinted on the Multiscale Magnetic Field

  • Authors: Jia-Wei Wang, Patrick M. Koch, Ya-Wen Tang, Gary A. Fuller, Nicolas Peretto, Gwenllian M. Williams, Hsi-Wei Yen, Han-Tsung Lee, Wei-An Chen

Jia-Wei Wang et al 2022 The Astrophysical Journal 931 .

  • Provider: AAS Journals

Caption: Figure 14.

Relative orientations between filaments and magnetic field (color scale), overlaid on the 850 μm intensity. The yellow and black segments are the magnetic field segments as shown in Figure 2. Within the central hub, the longer filaments tend to be either parallel or perpendicular to the local magnetic fields, except for the filaments near the “U-shape” magnetic field pattern where the field is more complex.

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