ASCL Code Record
[ascl:1806.019]
SYGMA: Modeling stellar yields for galactic modeling
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.
- Code site:
- https://nugrid.github.io/NuPyCEE/sygma.html https://github.com/NuGrid/NuPyCEE
- Described in:
- https://ui.adsabs.harvard.edu/abs/2018ApJS..237...42R
- Bibcode:
- 2018ascl.soft06019R
Preferred citation method:
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