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[ascl:1703.006] SNRPy: Supernova remnant evolution modeling

SNRPy (Super Nova Remnant Python) models supernova remnant (SNR) evolution and is useful for understanding SNR evolution and to model observations of SNR for obtaining good estimates of SNR properties. It includes all phases for the standard path of evolution for spherically symmetric SNRs and includes alternate evolutionary models, including evolution in a cloudy ISM, the fractional energy loss model, and evolution in a hot low-density ISM. The graphical interface takes in various parameters and produces outputs such as shock radius and velocity vs. time, SNR surface brightness profile and spectrum.

Code site:
http://www.quarknova.ca/#software https://github.com/denisleahy/SNRmodels
Appears in:
http://adsabs.harvard.edu/abs/2017arXiv170105942L http://adsabs.harvard.edu/abs/2017ApJ...837...36L
Bibcode:
2017ascl.soft03006L

ascl:1703.006
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