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Autor:
Zapartas, E, De Mink, SE, Van Dyk, SD, Fox, OD, Smith, N, Bostroem, KA, De Koter, A, Filippenko, AV, Izzard, RG, Kelly, PL, Neijssel, CJ, Renzo, M, Ryder, S
Many young, massive stars are found in close binaries. Using population synthesis simulations we predict the likelihood of a companion star being present when these massive stars end their lives as core-collapse supernovae (SNe). We focus on stripped
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e622dd243d38d0b9cf6672e404fcb9f7
