White dwarfs, each containing about as much mass as our Sun but packed into a volume about the size of Earth, are the endpoints of evolution for most stars. Tho

White dwarfs, each containing about as much mass as our Sun but packed into a volume about the size of Earth, are the endpoints of evolution for most stars. Tho

This engaging volume guides readers into the hearts of massive stars on a journey toward understanding one of the universe's most fascinating occurrences, a sup

The determination of stellar ages has been - and still is - crucial for the development of our understanding of the universe, and to constrain theoretical model