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White dwarf: Revision history

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25 January 2026

  • curprev 21:2221:22, 25 January 2026 DanteWashere talk contribs 609 bytes +609 Created page with "'''White dwarf''' is a compact stellar remnant formed after a low- or intermediate-mass star exhausts its nuclear fuel and expels its outer layers. It is characterized by high density and the absence of ongoing fusion reactions. White dwarfs are discussed in astrophysics, stellar evolution, and observational astronomy. == Status == White dwarfs are observed through optical, ultraviolet, and X-ray measurements. Models of their structure, cooling rates, and role in binar..."