Abstract: SYGMA (Stellar Yields for Galactic Modeling Applications) follows the ejecta of simple stellar populations as a function of time to model the enrichment and feedback from simple stellar populations. It is the basic building block of the galaxy code One-zone Model for the Evolution of GAlaxies (OMEGA, ascl:1806.018) and is part of the NuGrid Python Chemical Evolution Environment (NuPyCEE, ascl:1610.015). Stellar yields of AGB and massive stars are calculated with the same nuclear physics and are provided by the NuGrid collaboration.
Credit: Ritter, C.; Côté, B.; Herwig, F.; Navarro, J. F.; Fryer, C.
Preferred citation method: https://ui.adsabs.harvard.edu/abs/2018ApJS..237...42R
Reason: Updated code entry.