3D Binary

3D binary star:

Mass loss rate varies from 10-7 to 10-5 solar mass per year. An AGB star locates at the origin and the separation of two stars are 7.5 AU.

3Dcolor.gif​

3Dsideview.2.gif​

3Dtopview.gif​

From the side view, we can see BH accretion of the secondary star during the pulsation of the AGB star.

I think the tilting disk has gone. Since it is low temperature simulation and during the evolution we saw a flat plane of high density gas.

The simulation stuck due to "Restart Required"

​2.5D

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