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  2. Binary black hole - Wikipedia

    en.wikipedia.org/wiki/Binary_black_hole

    The star field behind the black holes is being heavily distorted and appears to rotate and move, due to extreme gravitational lensing, as space-time itself is distorted and dragged around by the rotating black holes. [1] A binary black hole (BBH), or black hole binary, is a system consisting of two black holes in close

  3. ChordPro - Wikipedia

    en.wikipedia.org/wiki/ChordPro

    The ChordPro (also known as Chord) format is a text-based markup language for representing chord charts by describing the position of chords in relation to the song's lyrics. ChordPro also provides markup to denote song sections (e.g., verse, chorus, bridge), song metadata (e.g., title, tempo, key), and generic annotations (i.e., notes to the ...

  4. List of most massive black holes - Wikipedia

    en.wikipedia.org/wiki/List_of_most_massive_black...

    The supermassive black hole at the core of Messier 87, here shown by an image by the Event Horizon Telescope, is among the black holes in this list.. This is an ordered list of the most massive black holes so far discovered (and probable candidates), measured in units of solar masses (M ☉), approximately 2 × 10 30 kilograms.

  5. Ultimate Guitar - Wikipedia

    en.wikipedia.org/wiki/Ultimate_Guitar

    Ultimate Guitar (Ultimate Guitar USA LLC), also known as Ultimate-Guitar.com or simply UG, is an online platform for guitarists and musicians, started on October 9, 1998 by Eugeny Naidenov [1] and based in San Francisco, US.

  6. BBH - Wikipedia

    en.wikipedia.org/wiki/BBH

    Main page; Contents; Current events; Random article; About Wikipedia; Contact us; Pages for logged out editors learn more

  7. Black hole - Wikipedia

    en.wikipedia.org/wiki/Black_hole

    A black hole with the mass of a car would have a diameter of about 10 −24 m and take a nanosecond to evaporate, during which time it would briefly have a luminosity of more than 200 times that of the Sun. Lower-mass black holes are expected to evaporate even faster; for example, a black hole of mass 1 TeV/c 2 would take less than 10 −88 ...

  8. Timeline of black hole physics - Wikipedia

    en.wikipedia.org/wiki/Timeline_of_black_hole_physics

    1972 — Jacob Bekenstein suggests that black holes have an entropy proportional to their surface area due to information loss effects; 1974 — Stephen Hawking applies quantum field theory to black hole spacetimes and shows that black holes will radiate particles with a black-body spectrum which can cause black hole evaporation

  9. Black Holes, Wormholes and Time Machines - Wikipedia

    en.wikipedia.org/wiki/Black_Holes,_Wormholes_and...

    Black Holes, Wormholes and Time Machines is a book by physicist Jim Al-Khalili, published in 1999. Al-Khalili talks about a range of modern science topics, from geometry to the theory of relativity. [1] [2] [3] [4]