16 octubre 2014
A new model is the first characterization of the progenitor for a hydrogen-deficient supernova. The model predicts that a bright hot star, which is the binary companion to an exploding object, remains after the explosion.Their findings have important implications for the evolution of massive stars.
http://feeds.sciencedaily.com/~r/sciencedaily/~3/4pnQRo-TqOo/141016192828.htm
