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Honours Student
Amanda Karakas
The sulfur anomaly in planetary nebulae and post-AGB stars
I will be testing nucleosynthesis models of AGB stars to see if they can explain observations of sulfur depletion in their end products (planetary nebulae).
As the computation will be performed at NCI, only storage for the results is requested. About 50-100 GB of storage space should be sufficient.
None.