Disk, Tidal Disruption and R Scultoris Project Updates

Discs From Tidally Disrupted Companions:

Animation: https://guidarellig.github.io/ThreeJupiterMassDisk.mp4

Tidal Disruption Simulations:

Goals →

1.) Investigate Bonnor-Ebert Sphere stability in a hot wind-tunnel

2.) Will a disk form from the cold tidally disrupted material?

3.) What is the fraction of material that forms a disk?

Just to mention: I wrote my own RK4 code in python that can modify the AGB profiles from MESA. Iterates over point mass, alpha, and central density, and integrates the pressure.

Animation: https://guidarellig.github.io/3MJ_2p1E10R.mp4

R sculptoris:

I am working with Zhuo to simulate the system R Sculptoris, This will be similar to the L2 Puppis Paper where we attempt to predict the binary parameters and generate synthetic images with RADMC-3D. As of now Zhuohas prepaired a module to run and I am sorting out how the refinement should work.

Animation: https://guidarellig.github.io/RsculpII.mp4

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