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SIMPLIFI—Study of Interstellar Magnetic Polarization: A Legacy Investigation of Filaments. I. Magnetically Guided Accretion onto the DR21 Ridge

  • Authors: Thushara G. S. Pillai, Jens Kauffmann, Juan D. Soler, Mark Heyer, Philip C. Myers, Laura M. Fissel, Dan Clemens, Koji Sugitani, Enrique Lopez-Rodriguez, Fumitaka Nakamura, Andrea Giannetti, Daniel Seifried, Paul F. Goldsmith, Helmut Wiesemeyer, Evangelia Ntormousi, Gabriel Franco, Stefan Reissl, Karl M. Menten

Thushara G. S. Pillai et al 2026 The Astrophysical Journal 1004 .

  • Provider: AAS Journals

Caption: Figure 6.

Outline of a magnetic field and cloud geometry consistent with the HAWC+ observations. Blue and magenta vertical arrows indicate the global structure of the magnetic field. The blue cylinder represents a dense cloud, such as the DR21 Main Ridge. The green layers represent a sheet that envelopes the dense cloud and is oriented perpendicular to the magnetic field. Panel (a) presents a view in which the observer is located toward the left of the figure; the line of sight in this model is nearly perpendicular to ﹩{\boldsymbol{B}}﹩. Gray cloudlets represent gas parcels following trajectories parallel to ﹩{\boldsymbol{B}}﹩ that accrete onto the sheet or the dense cloud, depending on the impact parameter of the field line they follow. Acceleration vectors span nonzero angles with the local field line for nonzero impact parameters. Panel (b) provides a rotated view closely aligned with the observer’s perspective.

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