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environment of black holes. In passing, this plasma is somehow charged so strongly that
                  it starts to emit visible light, forming two bright jets along the axis of rotation of the
                  black hole. Scientists have long been trying to answer the question: what and at what
                  moment does the plasma rays shine? (It is precisely these questions that correspond to
                  the effect of cavitation: the plasma begins to shine as soon as cavitation starts its active
                  action, amplified by  electromagnetism,  -  note Aubakir D.A.!). Thanks to the NASA
                  “NuSTAR” space telescope and the “ULTRACAM” camera,  scientists were able to
                  measure the distance (acceleration zone) that particles run through in plasma jets before
                  they “turn on” and become bright sources of light. In their work, the researchers studied
                  two “X-ray” binary systems in the Milky Way. Each of them consists of a black hole
                  and  a  normal  star  absorbed  by  the  companion. The  first  system, the  V404  Cygnus,
                  reached  its  maximum  brightness  in  June  2015.  At  that  moment,  she  produced  the
                  brightest flash that the scientist could fixing X-ray binaries in the 21st century.
















                                    Photo 3 - Black hole with accretion disk and stream of glowing
                                            hot gas. From the open resource of the specified site.

                        The second pair, GX 339-4, at the time of the observation of the luminary is only
                  1% of the expected. The star and the black hole in the GX 339-4 are much closer to each
                  other than in the Swan V404 system. Despite their difference, the systems showed the
                  same time delays (about one-tenth of a second) between the fixation of the “NuSTAR”
                  first  X-ray  and  “ULTRACAM”  visible  light.  “One  possible  explanation  is  that  the
                  physics of the jets is not determined by the size of the accretion disk, but depends on the
                  speed, temperature and other properties of the particles in them”, says Poshak Gandhi,
                  lead author of the study from the University of Southampton (UK). The most convincing
                  assumption, which explains the delay, is that X-ray light emits material that is very close
                  to the black hole. First, strong magnetic fields accelerate a part of the substance. This
                  leads to the fact that the particles collide at a velocity close to the speed of light, exciting
                  a plasma that eventually emits a stream of optical radiation. So, the formation of jets in
                  black holes: but at what point does the plasma start to glow? The answer to this question
                  lies in the delay between X-ray and optical radiation. By multiplying the delay time for
                  particle velocity, scientists determined the maximum distance traveled by them, which
                  turned out to be approximately 30,000 kilometers. The segment is a zone of internal
                  acceleration in which the plasma accelerates and “turns on”, emitting light (it includes


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