Image Details
Caption: Figure 14.
Snapshots of the 13CO channel maps at the systematic velocity for models with ﹩{\dot{M}}_{{\rm{in}}}=1{0}^{-8}\,{M}_{\odot }\,{{\rm{yr}}}^{-1}﹩ (top), 10−7 M⊙ yr−1 (middle), and 10−6 M⊙ yr−1 (bottom) after the cessation of infall. Streamer-induced kinematic signatures decay gradually, but their survival times increase with the mass infall rate.
© 2026. The Author(s). Published by the American Astronomical Society.