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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 3.

SOFIA/HAWC+ 214 μm Stokes I image of DR21 in grayscale and contours with overlaid analysis masks (colored boundaries) used to separate the Main Ridge from the system of subfilaments. Thin colored lines indicate the spines of the Main Ridge and subfilaments, as derived from the Herschel-based column density map. The red ellipse marks the outflow region near DR21 Main, excluded from this study. A magenta cross marks the approximate location of the dense core N56. A dashed blue line shows the location of the subfilament 1S-X.

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