1 code implementation • 20 Feb 2019 • Sambaran Banerjee, Krzysztof Belczynski, Christopher L. Fryer, Peter Berczik, Jarrod R. Hurley, Rainer Spurzem, Long Wang
We find that the SN material fallback causes the convection-asymmetry kick to effectively retain similar number and mass of BHs in clusters as for the standard, momentum-conserving kick.
Solar and Stellar Astrophysics Astrophysics of Galaxies High Energy Astrophysical Phenomena