White dwarf stars are remnants of low-mass stars that have exhausted their fuel and shed their outer layers, leaving behind a hot, compact core. These stars are incredibly dense, with a sugar-cube-sized amount of white dwarf material having a mass of about a ton. White dwarfs are made up of degenerate matter, meaning that their electrons are so tightly packed that they cannot move freely, and their density is supported by electron degeneracy pressure.
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Some potential sources for a White Dwarf PDF Archive include: White dwarf stars are remnants of low-mass stars