
Transient Butterflies: Fast Blue Optical Transients can be powered by Jet-Shocked Cocoons
FBOTs or butterflies? Today’s paper presents a new model to describe the emission from fast blue optical transients.
FBOTs or butterflies? Today’s paper presents a new model to describe the emission from fast blue optical transients.
How do neutron stars acquire such strong magnetic fields? Why do these fields differ between pulsars and magnetars? Today’s paper suggests that *convective dynamos* may be at play.
Today’s authors study an FRB in the M81 galaxy. Read on for what they find (spoiler: it’s not what we would expect!).
SUPERnova fail!
An asymmetric supernova shedding insight into the mystery of stellar death
The missing link in powering supernovae? Have a read and find out!