Image Details
Caption: Figure 7.
Similar to Figure 1 but for IRAS 04169. This figure shows a complex outflow structure that is difficult to classify as one of the three outflow types considered. The bottom-right panel shows the P–V diagrams perpendicular to the outflow axis at 4″ (middle right) and 8″ (bottom right) from the protostar.
© 2026. The Author(s). Published by the American Astronomical Society.