SYGMA: Modeling stellar yields for galactic modeling

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Ada Coda
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SYGMA: Modeling stellar yields for galactic modeling

Post by Ada Coda » Wed Jun 27, 2018 12:25 am

[c]SYGMA: Modeling stellar yields for galactic modeling[/c][/b]
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.

Site: https://github.com/NuGrid/NuPyCEE
https://ui.adsabs.harvard.edu/abs/2018ApJS..237...42R

Bibcode: 2018ascl.soft06019R

Preferred citation method: https://ui.adsabs.harvard.edu/abs/2018ApJS..237...42R

ID: ascl:1806.019
Last edited by Ada Coda on Sat Jul 13, 2019 4:08 pm, edited 1 time in total.
Reason: Updated code entry.

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