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posted by chromas on Wednesday September 12 2018, @08:08AM   Printer-friendly
from the dept.

Galaxy Punches Through Neighbor to Spawn Giant Ring of Black Holes

A giant ring of black holes has been discovered 300 million light-years away, offering new clues about what happens when galaxies collide. [...] The observed ring of black holes or neutron stars is believed to be the result of a galaxy collision. The galaxies were likely drawn together by gravity, and the gravitational force from one galaxy created waves in the gas surrounding its neighbor, which, in this case, is AM 0644. The ripples would have then caused the gas to expand or clump together in denser areas, triggering the birth of new stars.

"The most massive of these fledgling stars will lead short lives — in cosmic terms — of millions of years," representatives from the Chandra X-ray Observatory said in a statement. "After that, their nuclear fuel is spent, and the stars explode as supernovas, leaving behind either black holes with masses typically between about five to twenty times that of the sun, or neutron stars with a mass approximately equal to that of the sun." The black holes or neutron stars have close cosmic companions from which they siphon gas. This gas falls inward and is heated by friction, creating the bright X-rays detected by Chandra, according to the statement.

Also at Bad Astronomy.


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  • (Score: 2) by c0lo on Wednesday September 12 2018, @09:26AM (11 children)

    by c0lo (156) Subscriber Badge on Wednesday September 12 2018, @09:26AM (#733527) Journal

    This gas falls inward and is heated by friction

    Friction... with exactly what? What's there to rub against? Not like the black hole will have an atmosphere, is it?

    Are we talking about high speed collision between gas atoms?
    Are we talking about EM emmision of charged particles moving with acceleration (e.g. cyclotron radiation?)

    I can't imagine particles grinding at high speed against the black hole's horizon and sparking in the process.

    --
    https://www.youtube.com/watch?v=aoFiw2jMy-0 https://soylentnews.org/~MichaelDavidCrawford
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  • (Score: 0) by Anonymous Coward on Wednesday September 12 2018, @10:03AM

    by Anonymous Coward on Wednesday September 12 2018, @10:03AM (#733532)

    Internal friction of the gas.

  • (Score: 3, Informative) by RS3 on Wednesday September 12 2018, @12:54PM (3 children)

    by RS3 (6367) on Wednesday September 12 2018, @12:54PM (#733575)

    I can't imagine particles grinding at high speed against the black hole's horizon and sparking in the process.

    The gas atoms and molecules are increasingly compressed and collide as they fall into the black hole's gravitation. The forces and energies involved are indeed quite unimaginable.

    • (Score: 2) by c0lo on Wednesday September 12 2018, @01:40PM (2 children)

      by c0lo (156) Subscriber Badge on Wednesday September 12 2018, @01:40PM (#733587) Journal

      The gas atoms and molecules are increasingly compressed and collide as they fall into the black hole's gravitation.

      Like how much compressed?

      The forces and energies involved are indeed quite unimaginable.

      My imagination loves a challenge.

      (my point: thanks, but I'd really like some hard-science type of info)

      --
      https://www.youtube.com/watch?v=aoFiw2jMy-0 https://soylentnews.org/~MichaelDavidCrawford
  • (Score: 0) by Anonymous Coward on Wednesday September 12 2018, @12:57PM (3 children)

    by Anonymous Coward on Wednesday September 12 2018, @12:57PM (#733576)
    They grind against each other. Not everything is going to find itself in a trajectory heading into the black hole's event horizon, but all of the stuff near it is going to be accelerated to fantastic speeds by the black hole's gravity. And well, if you have stuff moving fast hitting other stuff moving fast, you get lots and lots of heat. One thing you really need to remember is that black holes aren't the all-sucking vacuum cleaners of the universe. The gravity for them is just the same as any other object of the same mass, just that if you happen to cross the event horizon it isn't possible to get back from beyond it.
    • (Score: 2) by c0lo on Wednesday September 12 2018, @01:59PM (2 children)

      by c0lo (156) Subscriber Badge on Wednesday September 12 2018, @01:59PM (#733593) Journal

      They grind against each other. Not everything is going to find itself in a trajectory heading into the black hole's event horizon, but all of the stuff near it is going to be accelerated to fantastic speeds by the black hole's gravity. And well, if you have stuff moving fast hitting other stuff moving fast, you get lots and lots of heat.

      So, high speed collision you say.

      The gravity for them is just the same as any other object of the same mass, just that if you happen to cross the event horizon it isn't possible to get back from beyond it.

      + Insightful on this one.
      Even though, to have high speed/high temp accretion with a lowish mass blackhole - just where from the energy is coming? The heating must happen in a narrow region close to the horizon.

      --
      https://www.youtube.com/watch?v=aoFiw2jMy-0 https://soylentnews.org/~MichaelDavidCrawford
      • (Score: 0) by Anonymous Coward on Wednesday September 12 2018, @02:29PM (1 child)

        by Anonymous Coward on Wednesday September 12 2018, @02:29PM (#733605)

        Even though, to have high speed/high temp accretion with a lowish mass blackhole - just where from the energy is coming?

        It comes from the same place that an asteroid falling to the earth gets its energy: gravitational potential energy. An object falling into a black hole will experience fantastic stresses as the gravitational potential is much higher at one end than the other, stretching it into spaghetti. Matter falling into the black hole forms an accretion disk, gets compressed and heated by the gravity, and radiates as a result. Since the matter will get fantastically hot in the process it'll become a superheated plasma, and naturally, charged particles accelerated by the black hole's gravity will also radiate in various ways (synchrotron radiation, brehmsstrahlung, etc.).

        • (Score: 2) by RS3 on Wednesday September 12 2018, @02:51PM

          by RS3 (6367) on Wednesday September 12 2018, @02:51PM (#733624)

          Is this happening on an atomic scale? And if you say "yes", then how close to the event horizon is atomic deformation beginning?

  • (Score: 3, Informative) by c0lo on Wednesday September 12 2018, @01:38PM

    by c0lo (156) Subscriber Badge on Wednesday September 12 2018, @01:38PM (#733585) Journal

    Heh, fascinating.

    X-RAY SPECTRA FROM MAGNETOHYDRODYNAMIC SIMULATIONS OF ACCRETING BLACK HOLES [iop.org]

    Since the initial discovery of the magnetorotational instability (MRI) by Balbus & Hawley (1991) over two decades ago, tremendous progress has been made in simulating astrophysical accretion disks.

    ...it was realized very early on that a great deal of the power of both stellar-mass black holes and active galactic nuclei (AGNs) is in the form of high-energy X-rays well above the thermal peak(...).

    Although it is now widely accepted that this hard flux comes from the inverse-Compton (IC) scattering of seed photons from the disk through a hot corona (...), we still know little or nothing about the origin or detailed properties of this corona. In classical disk theory there is no particular reason even to suppose such a corona exists.
    ...
    Recent advances in numerical simulation methods now allow us to approach this problem from an approach founded directly on disk dynamics. Angular momentum transport, the central mechanism of accretion, can be calculated directly, as it arises from correlations induced by orbital shear in MHD turbulence stirred by the MRI (Balbus & Hawley 1998). Moreover, the same magnetic fields essential to creating internal stresses automatically rise buoyantly above the dense regions of the disk and dissipate, creating a hot corona. Thus, the mechanisms treated by MHD simulations lead directly to physical processes that promise to explain coronal phenomenology.

    This is how the simulated black-hole disk corona looks/moves like [jhu.edu] - movie clip has some phenomena highlights.

    --
    https://www.youtube.com/watch?v=aoFiw2jMy-0 https://soylentnews.org/~MichaelDavidCrawford
  • (Score: 0) by Anonymous Coward on Wednesday September 12 2018, @05:07PM

    by Anonymous Coward on Wednesday September 12 2018, @05:07PM (#733713)

    You see, black hole is a stellar mass compacted to a several orders of magnitude smaller radius then the original star.

    Stars "ignite" through the similar process: gravitational attraction between center of star's mass and every single particle in its contents draws the particles closer to the center of the mass, and in the process, brings them closer together. Particles' total kinetic energy is increased through their loss of gravitational potential energy and they exchange their energy and momenta between themselves through collisions.

    With ample supply of interstellar gas and other matter (dust) around black hole, the same happens when it is drawn to the same radius around the center of the mass of black hole as they are inside a star - matter gets energetic, hot, and perhaps even starts to undergo nuclear fusion, creating even more energy in the process. Light and even some particles, the light ones as well as heavy element nuclei ones may even escape away from black hole (unless they are past its event horizon). But, unlike inside a star, there is less back pressure from the matter beneath them towards the periphery ("the bottom has fallen off").