meeting update

Rotating, supercritical Bonnor Ebert sphere forms a disk, protostar, and outflow.

Here is the density right before the outflow leaves the sphere:

right after:

Looks like a RT instability along jet axis.

Radial velocity (ignore the legend label — it's wrong) shows that the kernel is not directed outward, but beyond that, it is… Not sure why yet. Infall is happening in the disk though, which is as expected:

The temperature shows the outflow is decades larger than the core. This may need to be adjusted:

A movie of density can be found here:

​https://www.youtube.com/watch?v=rpUXAqMHjCs

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