SEVN PUBLIC VERSION

Download SEVN (Spera et al. 2015; Spera et al. 2017; Spera et al. 2019; Mapelli et al. 2019) from this link

https://gitlab.com/mario.spera/SEVN

Note that this version of SEVN does not support binary star evolution.

If you intend to use SEVN for a research paper, please include at least the following citations:

– Mapelli Michela, Spera Mario, Montanari Enrico, Limongi Marco, Chieffi Alessandro, Giacobbo Nicola, Bressan Alessandro, Impact of progenitor’s rotation and compactness on the mass of black holes, ApJ, in press, https://ui.adsabs.harvard.edu/abs/2019arXiv190901371M/

– Spera Mario, Mapelli Michela, Giacobbo Nicola, Trani Alessandro Alberto, Bressan Alessandro, Costa Guglielmo, Merging black hole binaries with the SEVN code,  2019, MNRAS, 485, 889, http://ui.adsabs.harvard.edu/abs/2019MNRAS.485..889S

– Spera Mario, Mapelli Michela, Very massive stars, pair-instability supernovae and intermediate-mass black holes with the SEVN code, 2017, MNRAS, 470, 4739,

http://ui.adsabs.harvard.edu/abs/2017MNRAS.470.4739S

– Spera Mario, Mapelli Michela, Bressan Alessandro, The mass spectrum of compact remnants from the PARSEC stellar evolution tracks, 2015, MNRAS, 451, 4086 , http://ui.adsabs.harvard.edu/abs/2015MNRAS.451.4086S