Image Details
Caption: Figure 3.
Synthetic images of the innermost region of disks observed with ALMA and ngVLA. Each row corresponds to the No-pileup (top), Fiducial (middle), and Extreme (bottom) model. The integration time is set to 10 hr. The observing beam size is denoted with a white-filled ellipse at the lower left in each panel.
© 2022. The Author(s). Published by the American Astronomical Society.