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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.


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.