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| Description: A Summary of Stellar Evolution (a) The evolution of isolated stars depends on their masses. The higher the mass, the shorter the lifetime. Stars less massive than about 8 solar masses can eject enough mass to become white dwarfs. High-mass stars can produce Type II supernovae and become neutron stars or black holes. The horizontal (time) axis is not to scale, but the relative lifetimes are accurate Picture Stats: Views: 8071 Filesize: 535.8kB Height: 900 Width: 1243 Source: https://biology-forums.com/index.php?action=gallery;sa=view;id=18636 |