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  2. PKS 2131-021 - Wikipedia

    en.wikipedia.org/wiki/PKS_2131-021

    PKS 2131-021 is a quasar and a BL Lacerate object, [2] producing an astrophysical jet. [ 3 ] lt is located in the constellation Aquarius and classified as a blazar , a type of active galactic nucleus whose relativistic jet points in the direction towards Earth .

  3. Andromeda–Milky Way collision - Wikipedia

    en.wikipedia.org/wiki/Andromeda–Milky_Way...

    The Milky Way and Andromeda galaxies each contain a central supermassive black hole (SMBH), these being Sagittarius A* (c. 3.6 × 10 6 M ☉) and an object within the P2 concentration of Andromeda's nucleus (1–2 × 10 8 M ☉). These black holes will converge near the centre of the newly formed galaxy over a period that may take millions of ...

  4. Binary black hole - Wikipedia

    en.wikipedia.org/wiki/Binary_black_hole

    Computer simulation of the black hole binary system GW150914 as seen by a nearby observer, during its final inspiral, merge, and ringdown. 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.

  5. Scientists Found the Speed Limit of Merging Black Holes

    www.aol.com/scientists-found-speed-limit-merging...

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  6. Humanity gets peek at what happens inside a black hole

    www.aol.com/humanity-gets-peek-happens-inside...

    Scientists have got a peek at what is happening inside of black holes. A new model – built on gravitational waves that were first detected almost 10 years ago – indicates what is going inside ...

  7. Stellar collision - Wikipedia

    en.wikipedia.org/wiki/Stellar_collision

    Any stars in the universe can collide, whether they are "alive", meaning fusion is still active in the star, or "dead", with fusion no longer taking place. White dwarf stars, neutron stars , black holes , main sequence stars , giant stars , and supergiants are very different in type, mass, temperature, and radius, and accordingly produce ...

  8. Gaia BH1 - Wikipedia

    en.wikipedia.org/wiki/Gaia_BH1

    The star and black hole orbit each other with a period of 185.59 days and an eccentricity of 0.45. The star is similar to the Sun , with about 0.93 M ☉ and 0.99 R ☉ , and a temperature of about 5,850 K (5,580 °C ; 10,070 °F ), while the black hole has a mass of about 9.62 M ☉ . [ 3 ]

  9. Neutron star merger - Wikipedia

    en.wikipedia.org/wiki/Neutron_star_merger

    When they finally meet, their merger leads to the formation of either a more massive neutron star, or—if the mass of the remnant exceeds the Tolman–Oppenheimer–Volkoff limit—a black hole. The merger can create a magnetic field that is trillions of times stronger than that of Earth in a matter of one or two milliseconds. [2]