Plan

  1. I discovered a mistake in the AGB star model (in the code). It is relevant to the optical depth. I will fix it this week.
  1. Due to the mistake, the mass loss rate was not correct. I think the mass loss rate is crucial in the formation of circumbinary disk. is somewhat small. If there could be a AGB wind, the formation of the circumbinary disk will be much more easier. ​Liljegren et al. (2016) did a detailed study on AGB wind recently. I will try their model.
  1. I will work with Jonathan to add the self-consistent mass loss calculation in AstroBEAR.
  1. Run 4 low res simulations (3au, 4au, 6au, 10au). May not finish all of them since it takes 24hrs to finish a 3au simulation.

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