Image Details
Caption: Figure 4.
Similar to Figure 1 but for BHR 71 IRS 1. This is an example of an outflow showing slow disk wind emission, where the outflow axis is inclined to the plane of the sky. The bottom-right panel shows the P–V diagrams perpendicular to the outflow axis at 3″ (middle right) and 6″ (bottom right) from the protostar.
© 2026. The Author(s). Published by the American Astronomical Society.