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[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:
http://nugrid.github.io/NuPyCEE/sygma.html https://github.com/NuGrid/NuPyCEE
Appears in:
http://adsabs.harvard.edu/abs/2017arXiv171109172R
Bibcode:
2018ascl.soft06019R

ascl:1806.019
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