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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 6.

Similar to Figure 1 but for IRAS 04166. This is an example of an outflow showing a combination of slow disk wind and wind-driven shell emission. The bottom-right panel shows the P–V diagrams perpendicular to the outflow axis at 1﹩\mathop{.}\limits^{\unicode{x02033}}﹩5 (middle right) and 3″ (bottom right) from the protostar.

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