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  2. WD J2147–4035 - Wikipedia

    en.wikipedia.org/wiki/WD_J2147–4035

    The white dwarf existed for 10.21 ±0.22 Gyrs, meaning the total age is 10.7 ±0.3 Gyrs. [1] Cold white dwarfs are often strongly affected by collision induced absorption (CIA) of hydrogen. This can lead to faint optical red and infrared brightness. These white dwarfs are also called IR-faint white dwarfs. WD J2147–4035 is however very red (r ...

  3. White dwarf - Wikipedia

    en.wikipedia.org/wiki/White_dwarf

    Sirius B, which is a white dwarf, can be seen as a faint point of light to the lower left of the much brighter Sirius A. A white dwarf is a stellar core remnant composed mostly of electron-degenerate matter. A white dwarf is very dense: in an Earth sized volume, it packs a mass that is comparable to the Sun.

  4. Carbon detonation - Wikipedia

    en.wikipedia.org/wiki/Carbon_detonation

    Carbon detonation or carbon deflagration is the violent reignition of thermonuclear fusion in a white dwarf star that was previously slowly cooling. It involves a runaway thermonuclear process which spreads through the white dwarf in a matter of seconds, producing a type Ia supernova which releases an immense amount of energy as the star is blown apart.

  5. Astronomers observe scar on white dwarf 'cannibal' star - AOL

    www.aol.com/news/astronomers-observe-scar-white...

    This white dwarf started its life as a star about twice the sun's mass, living a lifespan of perhaps 1.2 billion years before entering its death throes. Many white dwarfs have a debris disk ...

  6. Degenerate matter - Wikipedia

    en.wikipedia.org/wiki/Degenerate_matter

    Fowler described white dwarfs as composed of a gas of particles that became degenerate at low temperature; he also pointed out that ordinary atoms are broadly similar in regards to the filling of energy levels by fermions. [3] Milne proposed that degenerate matter is found in most of the nuclei of stars, not only in compact stars. [4]

  7. Hubble discovers hydrogen-burning white dwarfs enjoying ... - AOL

    www.aol.com/hubble-discovers-hydrogen-burning...

    White dwarfs are the slowly cooling stars that have cast off their outer layers during the last stages of their lives. Hubble discovers hydrogen-burning white dwarfs enjoying slow ageing Skip to ...

  8. Stellar evolution - Wikipedia

    en.wikipedia.org/wiki/Stellar_evolution

    For a star of 1 M ☉, the resulting white dwarf is of about 0.6 M ☉, compressed into approximately the volume of the Earth. White dwarfs are stable because the inward pull of gravity is balanced by the degeneracy pressure of the star's electrons, a consequence of the Pauli exclusion principle. Electron degeneracy pressure provides a rather ...

  9. Why Are People Mad About 'Snow White'? The Controversy ... - AOL

    www.aol.com/entertainment/why-people-mad-snow...

    A live-action version of Snow White and the Seven Dwarfs has been in development since at least 2016, but production didn’t kick off in earnest until 2021. In June of that year, Deadline ...