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Early Planet Formation in Embedded Disks (eDisk). XIX. Structures of Molecular Outflows

  • Authors: Anton Feeney-Johansson, Yuri Aikawa, Shigehisa Takakuwa, Nagayoshi Ohashi, Adele Plunkett, Jes K. Jørgensen, Hsien Shang, Zhi-Yun Li, Rajeeb Sharma, Woojin Kwon, Jeong-Eun Lee, Leslie W. Looney, Yao-Lun Yang, Mayank Narang, Itziar de Gregorio-Monsalvo

Anton Feeney-Johansson et al 2026 The Astronomical Journal 171 .

  • Provider: AAS Journals

Caption: Figure 10. Channel maps

The complete figure set (19 images) is available in the online journal.

Channel map of BHR 71 IRS 2. The stellar position is indicated by the cross at co-ordinates (0, 0). The axis of the jet is indicated by the vertical dashed line. The PA of the major axis of the dust continuum emission is indicated by the dashed line which intersects the vertical dashed line at the stellar position. Higher velocity channels, i.e., molecular jet, are described in S. Gavino et al. (2024).

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