I believe current models suggest that a low-metallicity stars (which are the ones who’s core can collage straight to a black hole, with no intermediate neutron star) will typically collapse with no supernova or other visible trace. High mass (> 90 SM) might lead to a GRB, but not a supernovae.
I believe current models suggest that a low-metallicity stars (which are the ones who’s core can collage straight to a black hole, with no intermediate neutron star) will typically collapse with no supernova or other visible trace. High mass (> 90 SM) might lead to a GRB, but not a supernovae.
You can follow the references at https://en.wikipedia.org/wiki/Failed_supernova & the supernova wikipedia page for the gory details.