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,
       author = {{Dabrowny}, Maciej and {Giacobbo}, Nicola and {Gerosa}, Davide},
        title = "{Modeling the outcome of supernova explosions in binary population synthesis using the stellar compactness}",
      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},
         year = 2021,
        month = dec,
       volume = {32},
       number = {4},
        pages = {665-673},
          doi = {10.1007/s12210-021-01019-8},
archivePrefix = {arXiv},
       eprint = {2106.12541},
 primaryClass = {astro-ph.HE},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2021RLSFN..32..665D},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

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