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White dwarf - Wikipedia, the free encyclopedia
A white dwarf, also called a degenerate dwarf, is a small star composed mostly of electron-degenerate matter. They are very dense; a white dwarf's mass is comparable to that of ...
White Dwarfs
An earth-sized white dwarf has a density of 1 x 10 9 kg/m 3. In comparison, the earth itself has an average density of only 5.4 x 10 3 kg/m 3. That means a white dwarf is 200,000 ...
White Dwarf (magazine) - Wikipedia, the free encyclopedia
White Dwarf is a magazine published by British games manufacturer Games Workshop. Initially covering a wide variety of fantasy and science-fiction role-playing and board games ...
white dwarf Facts, information, pictures | Encyclopedia.com ...
white dwarf in astronomy, a type of star that is abnormally faint for its white-hot temperature (see mass-luminosity relation ). Typically, a white...
White Dwarfs - Introduction
A low or medium mass star (with mass less than about 8 times the mass of our Sun) will become a white dwarf. A typical white dwarf is about as massive as the Sun, yet only ...
White Dwarf Research Corporation
A non-profit organization dedicated to scientific research and public education
White Dwarf
White Dwarf is a weird mix of game concepts like that of Katamari Damacy and several
White Dwarfs and Electron Degeneracy
White Dwarf When the triple-alpha process in a red giant star is complete, those evolving from stars less than 4 solar masses do not have enough energy to ignite the carbon fusion ...
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SFGate: Day in PicturesSan Francisco Chronicle... nuclear fuel exhausted, the sun-like star's life comes to a close as its outer layers are ejected, and its core becomes a cooling, fading white dwarf. ... |
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Nova Explosion Reveals Gamma RaysPhotonics.comThe explosion occurs when a white dwarf ignites in an enormous thermonuclear explosion. The newly detected explosion is equivalent to about 1000 times the ... |
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NASA Hubble Space Telescope Daily Report #5174Space Ref (press release)... hook stars are very likely the progeny of stars that undergo extensive internal mixing during a late helium core flash on the white dwarf cooling curve. ... |
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