Another type produces oxygen-rich remnants; that type, the core-collapse type, is responsible for the creation of the Crab Nebula.
One of these phenomena discovered in 2006 is a leading candidate to be the first-discovered pair-instability type of them. Another type produces oxygen-rich remnants; that type, the core-collapse type, is responsible for the creation of the Crab Nebula. The thermonuclear type of these phenomena, also known as Type Ia (ONE-A), occurs in stars that have a mass less than one point four times that of the sun; that limit is known as the Chandrasekhar limit. For 10 points, name these massive explosions in which a star blows itself up.
One of these phenomena discovered in 2006 is a leading candidate to be the first-discovered pair-instability type of them.
supernovae