Figure 6.
Surface density profiles of an evolving protoplanetary disc around a 0.1$\, {\rm M}_{\odot }$ star undergoing Inside-Out with Continued Accretion (IO-A) evolution throughout the disc lifetime. The uppermost blue line shows the initial disc profile, while the black line shows the last disc output before the disc had fully dispersed. The surface density is shown in intervals of intervals of 0.05 Myr.

Surface density profiles of an evolving protoplanetary disc around a 0.1|$\, {\rm M}_{\odot }$| star undergoing Inside-Out with Continued Accretion (IO-A) evolution throughout the disc lifetime. The uppermost blue line shows the initial disc profile, while the black line shows the last disc output before the disc had fully dispersed. The surface density is shown in intervals of intervals of 0.05 Myr.

Close
This Feature Is Available To Subscribers Only

Sign In or Create an Account

Close

This PDF is available to Subscribers Only

View Article Abstract & Purchase Options

For full access to this pdf, sign in to an existing account, or purchase an annual subscription.

Close