Image Details
Caption: Figure 1.
Formation and evolution of the disk. Top: gas surface densities (in log g cm−2) for the inner 200 au of the disk are shown at 13, 21, 30, 40, 50, and 60 kyr after protostellar birth in (a)–(f). Bottom: star and disk gas masses after the birth of the protostar (g) and evaporated and remaining dust masses in the disk (h).
© 2026. The Author(s). Published by the American Astronomical Society.