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A Tale of Three Tails: A Misaligned Streamer and Mysterious Structures around [BHB2007]-1

  • Authors: Aashish Gupta, Antonio S. Hales, L. Ilsedore Cleeves, Felipe Alves, Trisha Bhowmik, Nicolás Cuello, Josep M. Girart, Zhi-Yun Li, Anna Miotello, Zhaohuan Zhu, Alice Zurlo

Aashish Gupta et al 2026 The Astrophysical Journal 998 .

  • Provider: AAS Journals

Caption: Figure 3.

Intensity-weighted velocity (moment 1) maps of all three CO isotopologue emission lines imaged for this analysis: CO (2–1) (left), 13CO (2–1) (center), and C18O (2–1) (left). The horizontal gray lines in the bottom-left corners represent a length scale of 1000 au, and the pink ellipses in the bottom-right corners represent the beam size. Black contours denote the continuum emission (5σ) from the protoplanetary disks. The locations of structures A, B, and C and the nearby source BHB2 are marked on the maps.

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