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[ascl:2307.035] binary_c: Stellar population synthesis software framework

The binary_c software framework models the evolution of single, binary and multiple stars, including stellar evolution and nucleosynthesis. Stellar evolution includes wind mass loss, rotation, thermal pulses, magnetic braking, pre-main sequence evolution, supernovae and kicks, and neutron stars; binary-star evolution includes mass transfer, gravitational-wave losses, tides, novae, circumbinary discs, and merging stars. binary_c natively includes nucleosynthesis, and, as it is designed for stellar population calculations, it is lightweight and versatile. binary_c works in standalone, virtual and HPC environments, and its support software contains tools for development and data analysis. A version in Python, binary_c-python (ascl:2307.036), is also available.

Code site:
https://gitlab.com/binary_c https://binary_c.gitlab.io/
Used in:
https://ui.adsabs.harvard.edu/abs/2015A%26A...581A..62A https://ui.adsabs.harvard.edu/abs/2018Galax...6...97I
Described in:
https://ui.adsabs.harvard.edu/abs/2004MNRAS.350..407I
Bibcode:
2023ascl.soft07035I

Views: 828

ascl:2307.035
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