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Introduction to SYGMA

The Stellar Yields for Galactic Modeling Applications (SYGMA) module allows to follow the ejecta of simple stellar populations as a function of time.
For the access and introduction to the SYGMA web interface, see Web Interface.


Notes:

Stellar yields of AGB and massive stars are calculated with the same nuclear physics and are provided by the NuGrid collaboration. The interface is hosted by NuGrid's WENDI platform.