Time-Evolution Images of the Hypergiant RW Cephei During the
Re-brightening Phase Following the Great Dimming
Time-Evolution Images of the Hypergiant RW Cephei During the
Re-brightening Phase Following the Great Dimming
Stars with initial masses larger than 8 solar masses undergo substantial mass loss through mechanisms that remain elusive. Unraveling the origins of this mass loss is important for comprehending the evolutionary path of these stars, the type of supernova explosion and whether they become neutron stars or black hole remnants. …