Titlebook: Unlocking the Secrets of White Dwarf Stars; Hugh M. Van Horn Book 2015 Springer International Publishing Switzerland 2015 Dense Mass Stars

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1614-659X the universe.Places the advances in our understanding of whi.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. Thousands of these faint objects have now been discovered, though only a century a

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The First Clues, now call white dwarfs. Although he recognized that his finding was important, neither he nor any other scientist in the early nineteenth century had the remotest idea that dramatic advances in science and technology and a revolution in fundamental physics would be required before these stars could

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Star Power,energy needed to supply the prodigious power output of the stars. Release of chemical energy, such as the burning of a lump of coal, was easily shown to be inadequate. The heat produced by complete combustion of a lump of coal would release only 2–3?×?10. erg g., sufficient to maintain the current l