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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 11. Channel maps and the PV diagrams

The complete figure set (11 images) is available in the online journal.

(a) The velocity channel map, (b) the PV diagram along the outflow axis, and (c) the PV diagrams perpendicular to the outflow axis of the blueshifted outflow of IRAS 16544-1604. The positions of the P–V cuts are indicated in the channel map in the top right of (c). The distance in arcseconds of the P–V cut from the source along the jet axis is indicated in the top right of each P–V diagram. The white contours in the PV diagrams depict 4σ and 5σ. The feature categorized as a wind-driven shell is fitted with a simple model described by Equation (1), which is indicated by the orange lines.

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