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A Multiscale Picture of the Magnetic Field and Gravity from a Large-scale Filamentary Envelope to Core-accreting Dust Lanes in the High-mass Star-forming Region W51

  • Authors: Patrick M. Koch, Ya-Wen Tang, Paul T. P. Ho, Pei-Ying Hsieh, Jia-Wei Wang, Hsi-Wei Yen, Ana Duarte-Cabral, Nicolas Peretto, Yu-Nung Su

Patrick M. Koch et al 2022 The Astrophysical Journal 940 .

  • Provider: AAS Journals

Caption: Figure 7.

Local magnetic field strength maps (bottom row) derived from the stability and collapse criterion given in Equation (2). Separately displayed are the measurable input parameters ﹩\sin \omega ﹩ (top row) and ∣ g loc∣ (middle row; arbitrary units) for W51 e2 (left column) and e8 (right column).

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