On the desert between neutron star and black hole remnants

R. Caimmi
2018 Applied Mathematical Sciences  
< ∼ M/m < ∼ 4) BH formation are shortly discussed. Whether the desert between NS and BH remnants could be ascribed to biases and/or selection effects, or related to lack of formation channels, still remains an open question. To this respect, increasingly refined theoretical and observational techniques are needed.
doi:10.12988/ams.2018.811161 fatcat:azrdqnipmbatpmhqk3vph347cy