Modeling the outcome of supernova explosions in binary population synthesis using the stellar compactness. Dabrowny, M., Giacobbo, N., & Gerosa, D. *Rendiconti Lincei. Scienze Fisiche e Naturali*, 32(4):665-673, December, 2021. doi bibtex @article{2021RLSFN..32..665D,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {https://ui.adsabs.harvard.edu/abs/2021RLSFN..32..665D},
archiveprefix = {arXiv},
author = {{Dabrowny}, Maciej and {Giacobbo}, Nicola and {Gerosa}, Davide},
doi = {10.1007/s12210-021-01019-8},
eprint = {2106.12541},
journal = {Rendiconti Lincei. Scienze Fisiche e Naturali},
keywords = {Stars: evolution, Stars: supernovae, Black-hole physics, Gravitational waves, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Solar and Stellar Astrophysics, General Relativity and Quantum Cosmology},
month = dec,
number = {4},
pages = {665-673},
primaryclass = {astro-ph.HE},
title = {{Modeling the outcome of supernova explosions in binary population synthesis using the stellar compactness}},
volume = {32},
year = 2021,
bdsk-url-1 = {https://doi.org/10.1007/s12210-021-01019-8}}

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