Image Details
Caption: Figure 4.
The evolution of the radius (left) and kinetic energy (right) as a function of time from our equipartition analysis, assuming a single outflow is launched into the CNM around the time of optical discovery. The blue and red filled circles indicate the parameters for a spherical homogeneous and a collimated conical outflow, respectively.
© 2025. The Author(s). Published by the American Astronomical Society.