Download SEVN (Spera et al. 2015; Spera et al. 2017; Spera et al. 2019; Mapelli et al. 2019) from this link.
In order to have access to the repository, you should ask us to invite you. 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, 2020, 888, 76, https://ui.adsabs.harvard.edu/abs/2020ApJ…888…76M/abstract
– 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,
– 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