Image Details
Caption: Figure 1.
Segmentation results demonstrating superbubbles isolated from the input density (n) cube using our proposed tracking framework. The upper row features a supernova remnant case at t = 191.8 Myr, while the lower row shows a superbubble identified at t = 213.0 Myr in the same simulation.
© 2026. The Author(s). Published by the American Astronomical Society.