Figure 7
Final gas density distribution at a cluster age of 250 Myr. Superposed as blue dashed lines are the two limiting curves for the range of possible surface density distributions as determined from MIDI observations (Kishimoto et al. 2009).

Final gas density distribution at a cluster age of 250 Myr. Superposed as blue dashed lines are the two limiting curves for the range of possible surface density distributions as determined from MIDI observations (Kishimoto et al. 2009).

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