The explodability criterion: How to make a star go supernova
Today’s authors present some new insights into how stars explode!
Today’s authors present some new insights into how stars explode!
Today’s paper delves into the inert black hole binary VFTS 243 and what it can tell us about stellar death.
The origin of dim supernovae known as Ca-rich transients is still not well-understood. Could it be that these rare events are set off by an encounter between a white dwarf and a primordial black hole?
This black hole could have been born without any bright supernova explosion, emitting nothing but a few neutrinos in its formation. Find out how we can tell in today’s paper!
Who’s behind this cosmic mystery of stellar proportions? Read on to uncover the truth.
The first (and last) time we observed neutrinos from a supernova was 40 years ago. Are we ready to understand what the next supernova neutrino will tell us?